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453 Sentences With "near side"

How to use near side in a sentence? Find typical usage patterns (collocations)/phrases/context for "near side" and check conjugation/comparative form for "near side". Mastering all the usages of "near side" from sentence examples published by news publications.

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CE3 landed on the near side of the moon in 2013.
Hoffman's one-timer found the near side of the net, which was wide open.
Trockeck scored the goal from a bad angle, beating Kuemper to the near side.
But Jung, who takes the corner, curls it into the near-side goal netting.
It is possible that the far side of the moon was originally the near side.
Chang'e 3 landed on the Moon's near side, but it stopped functioning shortly after landing.[NASA]
The puck dribbled to the near side of the net and went just wide of the post.
"More and more in the NBA, the near side coverage is blocked to the viewer," Corrigan added.
The near side is covered with maria, or ancient lava flows; the far side has almost none.
But of course it's just fine to cross one if the dashes are on the near side.
The far side is also considerably more mountainous than the near side for reasons not yet understood.
The portion we're privileged to view is a northeastern region of the near side of the moon.
Dozens of spacecraft have observed the near side of the Moon and six have landed people on it.
China's first lunar probe, known as Chang'e-3, landed on the near side of the moon in 2013.
And when the near side of the moon is dark, the far side is awash in bright sunshine.
That makes the far side much lighter, much older and much more heavily cratered than the near side.
Image: CNSAAdditionally, most of the samples taken by missions to the near side of the Moon seem to contain traces from some cataclysmic collision that created the near side of the Moon's Mare Imbrium (the left eye, if you imagine the Moon, viewed from the Northern Hemisphere, as a face).
He curled one back to the near side of the goal area and Messi was there with his left foot.
China's first lunar lander, the Chang'e-3, completed a journey to the near side of the moon five years ago.
Chang'e 1 and 2 orbited the Moon, and Chang'e 3 was a lunar lander and rover on the Moon's near side.
That lander, part of the Chang'e-3 mission, went to the Moon's near side, the one we see at all times.
Campbell's shot from outside the left circle ricocheted off Sabres defenseman Rasmus Ristolainen and into the near side of the net.
This data showed that the far side crust was about 215 kilometers (2000 miles) thicker than the crust on the near side.
A passing sequence between defenseman Sami Vatanen and Taylor Hall resulted in an unmarked Hughes receiving the puck on the near side.
Landing on the near side of the Moon is easy (relatively speaking) because there's nothing blocking communication signals between the two worlds.
André-Pierre Gignac tracked a ball down the near side, but slipped as he was cutting to the middle of the field.
If it was still on the near side of the wall, Betts had to be given his chance to catch it unmolested.
Some astronomers suspect the dichotomy arises because the crust on the near side is much thinner than that of the far side.
That would make it easier for magma to emerge on the near side, explained Briony Horgan, a planetary scientist at Purdue University.
And when the Sun lights up the far side of the Moon, the near side is dark and we see a new Moon.
Huberdeau took a pass from Keith Yandle and scored on the near side as Barkov skipped out of the way of the puck.
China's first lunar lander and rover, Chang'e-3, landed on the near side of the moon five years ago, but faced numerous mechanical issues.
The Indian Space Research Organization (ISRO) will attempt to land the Vikram probe on the Moon's near side in the unexplored south polar region.
The far side of the moon is tidally locked to always face away from the Earth, and is even more cratered than the near side.
Barca had sustained pressure in front of the Celtic net for some time before the ball finally got to Neymar streaking down the near side.
They were battling under the near side of the rim and then Love just let him go to the other side to get a clean rebound.
There's the standard grabbing of the near side wrist and trying to smash it down with his knee or hips, in order to feed it through.
NASA knows precisely what color the moon's near side is, so when it wants to calibrate HiRise, it points it at the moon and takes some images.
Humans have landed dozens of probes on the near side of the Moon, but Chang'e 4 is the first spacecraft to achieve a touchdown on the far side.
Raad's hyperawareness of the invisible forces of greed keeps his impersonation of a madman ever attuned to the mystical vibrations of power on the near side of fatuousness.
When he came back around to the near side of the moon he used a telescope to search for his comrades on the surface but couldn't spot them.
He could threaten a kimura , which would probably be impossible to finish on the near side arm, and the opponent would just forget their guard and let him mount.
The tour kicks off on the western edge of the Moon, at the Mare Orientale (aka the Orientale Basin), where the sunlit near side meets the shadowy far side.
The face of the "man in the moon" on the near side is so noticeable because it's composed of dark areas, which stand out against the light lunar soil.
This near side of the Moon is the only region that we've landed on gently, because there's a direct line of sight with Earth, enabling easier communication with ground control.
Duchene took a second to settle a puck that was on edge and then whistled a high shot to the near side, past Luongo just 275 seconds into the game.
The intelligence officers—five conservatively dressed men, just on the near side of middle age—directed theirs from a living room filled with vintage movie posters, overlooking a burrito shop.
Only China, the former Soviet Union and the United States have sent spacecraft to the surface of the moon, though previous explorations have landed on the near side that faces Earth.
Beresheet is slated to reach its destination on the near-side of the moon in mid-April following a two-month journey through 5853 million miles (6.5 million km) of space.
Some of the resultant craters penetrated the lunar crust may reveal more readily the range of minerals and resources on the lunar surface beyond anything we have seen on the near side.
United were moving quickly on the counter and the ball eventually found its way to Cameron Borthwick-Jackson, who a sent a cross in from the near side into the penalty area.
Athanasiou showed some nifty wheels, skating from behind the net around to the right faceoff circle, where he snapped a shot that beat Braden Holtby near side to tie the score at 1.
When a fighter passes the near side arm underneath his opponent (in this case Knights' right arm) he also removes a block stopping his opponent from walking around him to north-south position.
The far side of the moon has been impacted over millions of years by meteors and is far more rugged than the smoother lava surfaces on the near side that we see routinely.
Since it takes the Moon roughly the same amount of time to spin around its axis as it does to orbit the Earth, we only see one half of the Moon: its near side.
The Pittsburgh-based Astrobotic, which is backed by the Space Angels Network, was awarded $79.5 million to fly up to 14 payloads to Lacus Mortis, a large crater on the near side of the moon by July 2021.
But all these non-Chinese efforts will land on the Moon's Earth-facing near side, and thus within the solicitous sight of Earthbound controllers—just as all previous lunar landings, whether American, Soviet or, since 2013, Chinese, have been.
This wonderful group did it, and landed in a place that we've never been before... the far side seems to be so different from the near side, and they could be recording so much information that we're still missing.
If all goes according to plan, Beresheet, about the size of a dishwasher, will arrive on the near-side of the moon in mid-April following a two-month journey through 4 million miles (6.5 million km) of space.
Its top speed is around 200 meters per hour, or just over one-eighth of a mile per hourBack in 2013, China deployed its Yutu rover, or Jade Rabbit 1, on the Moon's near side as part of the Chang'e 3 mission.
Between his forcing butterfly half and driving over the hook, using the near side underhook pass from traditional half, and smash passing into what he termed 'dope mount', Penn had twice as many routes to mount as he would need in any situation.
In a paper published in the journal Science in 2015, a different group of Chinese researchers described a complex geology of nine distinct layers below Mare Imbrium, a lava plain on the moon's near side where China's earlier mission, Chang'e-3, had landed.
Just 31 seconds later, Sieloff, a defenseman who was playing his first NHL game, threw a backhand shot toward the Minnesota net from the right circle that bounced over Kuemper's glove and just inside the near-side post for what turned out to be the game winner.
" Although we eventually learn what she did to her teacher, we never tire of Nadine's voice, which seems to hover on the near side of madness: "There was something freeing, something rapturous, even, about that moment when my hand came down and broke through his skin.
The lead author of the new study, Zhu Meng-Hua of the Space Science Institute at Macau University of Science and Technology, had a hunch the near side-far side asymmetries were the result of celestial collision after looking at data gathered in 2500 by the Gravity Recovery and Interior Laboratory (GRAIL) mission.
Specifically, the near side-far side asymmetry was shown to be caused by a large object measuring 780 kilometers (480 miles) in diameter hitting the Moon's nearside at 22,550 km/h (33,000 mph) or a slightly smaller object at 720 kilometers across (450 miles) at a higher speed of 24,500 km/h (15,000 mph).
The Chang'e-4 probe is China National Space Administration part of a series of missions designed to explore the surface of the moon, which started in 2007 with the Chang'e-1 orbiter, and was followed in 2010 by the Chang'e-2 orbiter, and the Chang'e-3 lander, which successfully touched down on the near side of the moon in 2013.
Rookie Jack Hughes scored his first NHL goal, and Mackenzie Blackwood recorded his first shutout of the season as the New Jersey Devils skated to a 1-0 win over the Vancouver Canucks on Saturday afternoon in Newark, N.J. A passing sequence between defenseman Sami Vatanen and Taylor Hall resulted in an unmarked Hughes receiving the puck on the near side.
Partial and total eclipses together with simply partial last for up to about six hours without having totality in all parts of the near side and a very small part of the far side next to the near side. Standalone partial and total eclipses between partial eclipses can last up to 3.5 hours.
In 2009, the IAU named a lunar impact crater located on the lunar near side near the northern pole after Gore.
Hubble views of Copernicus crater (inset), showing its location on the near side Copernicus is named after the astronomer Nicolaus Copernicus. Like many of the craters on the Moon's near side, it was given its name by Giovanni Riccioli, whose 1651 nomenclature system has become standardized.Whitaker, Ewan A (1999). Mapping and Naming the Moon (Cambridge University Press), p.61.
Return to near side, and pass the loose end of running rope around the forward end, bottom and finally rear end of kyack.
On its north-west edge lies the 32 km wide Aristarchus ray crater, the brightest feature on the Near side of the Moon.DK Space Encyclopedia: The Near Side of the Moon Also, the more-prominent ray-crater Copernicus lies within the eastern edge of the mare, distinctly with its bright ray materials sprawling over the darker material. On the northern edge of Oceanus Procellarum lies Sinus Roris.
Only 1% of the surface of the far side is covered by maria, compared to 31.2% on the near side. According to research analyzed by NASA's Gravity Recovery and Interior Laboratory (GRAIL) mission, the reason for the difference is because the Moon's crust is thinner on the near side compared to the far side.Universe Today The dark splotches that make up the large lunar maria are lava-filled impact basins that were created by asteroid impacts about four billion years ago. Though both sides of the Moon were bombarded by similarly large impactors, the near side hemisphere crust and upper mantle was hotter than that of the far side, resulting in the larger impact craters.
Lunar eclipses occur only at a full moon and often cause a reddish hue on the near side of the Moon. This full moon has been called a blood moon in popular culture.
LRO image Promontorium Taenarium is a headland on the near side of the Moon. It is located in the eastern end of Mare Nubium. Its length is about 70 km. Its coordinates are .
Water pump mounted on the front of the timing gear case delivering into a gallery pipe along the near side of the engine with eight separate feeds into the cylinder block below the exhaust ports.
Promonontorium Kelvin, a small mountain range narrowly connected to Rupes Kelvin. Lunar Orbiter 4 photo. Promontorium Kelvin is a headland on the near side of the Moon. It is located in the southeast of the Mare Humorum.
October 17, 1905. Witte, Rosen, Plancon; and the Japanese at near side of table are Adachi, Ochiai, Komura, Takahira, Satō. The large conference table is today preserved at the Museum Meiji Mura in Inuyama, Aichi Prefecture, Japan.
Meanwhile, some eclipses are shorter when the Earth is slightly further away from the Moon. On Earth, the Moon is seen with its apparent diameter smaller than the Sun's. Unlike the Earth, where its eclipses start and end at a different place, all of the Moon's solar eclipses begin in the westernmost parts of the near side and end in the easternmost parts of the near side. Solar eclipses starting near and within the polar areas are always partial, while solar eclipses starting at or within the equator are always total.
Detail map of Mare Imbrium's features. Montes Apenninus is marked with a "K". Montes Apenninus are a rugged mountain range on the northern part of the Moon's near side. They are named after the Apennine Mountains in Italy.
The Beresheet lunar lander's target landing destination was within Mare Serenitatis, a vast volcanic basin on the Moon's northern near side. Despite the failure, the mission represents the closest a private entity has come to a soft lunar landing.
Oblique view of Kunowsky from Apollo 12. NASA photo. Kunowsky is a small lunar impact crater on the Mare Insularum, in the western half of the Moon's near side. It is named after the German astronomer Georg Karl Friedrich Kunowsky.
Fountain near side entrance of Kruidtuin A greenhouse of the orangery The Hortus Botanicus Lovaniensis (Dutch: Kruidtuin) is a botanical garden in Leuven, Belgium, dating from 1738. It is situated in the city centre and has an extent of 2.2 hectares.
On the near side the Earth and its magnetic field partially shield the surface from the solar wind during each orbit. But the far side is fully exposed, and thus should receive a somewhat greater proportion of the ion stream.
Aerial view of the Guadalupe River and Tasman Drive, with Guadalupe River Trail on far (east) side in San Jose and Ulistac Natural Area on near side in Santa Clara The Guadalupe River Trail runs along of the river bank.
Sparking plugs are easily accessed. The vertically driven make and break and distributor is on the off side in front of the generator. Inlet and exhaust manifolds are cast together and mounted on the near side. There is an air cleaner.
Solar eclipses on the Moon are caused when the planet Earth passes in front of the Sun and blocks its light. Viewers on Earth experience a lunar eclipse during a solar eclipse on the moon. These solar eclipses are only seen in the near side portion and smaller parts of the far side where Earth is seen during librations, these areas of the moon making up the visible portion of the Moon. Eclipses there are seen during the lunar sunrise and sunset and extend to the furthermost areas of the near side but mainly not in the polar areas of the Moon.
About ninety-one percent of the far side never experiences solar eclipses as the Earth is never seen there because the limit of the view of the planet during librations is about eight degrees within the near side. Eclipses are generally not seen in the fringes of the near side, within the far side, or in the lower and most of the middle parts. Around it, it is not seen in the lower parts. In that location and around it, the eclipses are never seen in most crater hollows or some of the lowest parts of some crater hollows.
The near side of the moon, from where energy would be beamed to Earth, according to the Luna Ring project. Luna Ring is a speculative engineering project which consists in a series of solar generators, disposed around the equator of the Moon, that could send the generated electric energy back to the Earth via microwaves from the near side of the Moon. The project was proposed by Japanese construction firm Shimizu Corporation, after the 2011 Tōhoku earthquake and tsunami destroyed the Fukushima Daiichi Nuclear Power Plant, creating public opposition against nuclear electric energy. Until then, Japan had relied heavily on nuclear power.
The crater has a notable central peak at the midpoint of the interior floor. A cleft-like feature crosses the southern rim and continues to the south. Behaim is similar in appearance to Alpetragius crater on the near side, although Behaim is larger.
California State Parks of San Luis Obispo Coast: El Moro Elfin Forest . accessed 5.25.2012 A panoramic view of Estero bay (far side of sandspit), Morro Bay (near side of sandspit), Los Osos, Baywood Park, Chorro Valley, and Hollister Peak, from Black Hill.
The crankshaft runs in two large bearings. Timing is by chain. The valves are at the side and worked by tappets acting directly on a large-diameter two-bearing camshaft. Tappets are on the near side and may be accessed for regulation.
Aerial view of Ulistac Natural Area, along the near side of the Guadalupe River The Ulistac Natural Area is a 40-acre volunteer-maintained natural area within the original rancho, between Lick Mill Blvd. and the Guadalupe River, showcasing seven distinctive natural habitats.
The knee closest to the puck remains vertical next to the goal post. The advantage is on coverage against quick shots to the near side of the net, while still covering the option to track passes to the front of the goal mouth.
On the far side of the figure, the return current flows from the rotating arm through the far side of the rim to the bottom brush. The B-field induced by this return current opposes the applied B-field, tending to decrease the flux through that side of the circuit, opposing the increase in flux due to rotation. On the near side of the figure, the return current flows from the rotating arm through the near side of the rim to the bottom brush. The induced B-field increases the flux on this side of the circuit, opposing the decrease in flux due to r the rotation.
Because line-of-sight tracking was required for this experiment, only the near-side gravity field could be estimated using this Doppler method. The experiment was a byproduct of the spacecraft S band tracking, and so has no listed weight or power requirements. The experiment was designed to give the near-side gravity field with a surface resolution of and precision of 5 mGal (0.05 mm/s²) in the form of spherical harmonic coefficients to degree and order 60. In the extended mission, in which the spacecraft descended to an orbit with an altitude of and then to , this resolution was expected to improve by a factor of 100 or more.
Oblique view of northern Mare Nubium from Apollo 16. Volcanic feature in Mare Nubium Mare Nubium (Latin nūbium, the "sea of clouds") is a lunar mare in the Nubium basin on the Moon's near side. The mare is located just to the southeast of Oceanus Procellarum.
The lunar crater Morley on the near side was named for him. The Morley Elementary School in West Hartford, Connecticut, was also named for him, as was the Morley Scientific Laboratory on the Williams College campus. His house in West Hartford was made a National Historic Landmark in 1975.
Japan-Russia Treaty of Peace, or "Treaty of Portsmouth", September 5, 1905. Diplomatic Archives of the Ministry of Foreign Affairs of Japan. Witte, Rosen, Plancon; Japanese (near side) Adachi, Ochiai, Komura, Takahira, Satō. The conference table is today preserved at the Museum Meiji-mura in Inuyama, Aichi Prefecture, Japan.
This was the first small car to have the Daimler fluid flywheel transmission.The Olympia Show. The Times, Saturday, 14 October 1933; pg. 7; Issue 46575 The preselection finger and thumb lever was just under the steering wheel on the near side and so worked by the left hand.
Hill crater (lower right) from Apollo 15. NASA photo. Oblique view of Carmichael also from Apollo 15 Carmichael is a lunar impact crater that is located along the eastern edge of the Sinus Amoris, in the northeastern quadrant of the Moon's near side. Its diameter is 20 km.
Other large impact basins, such as the maria Imbrium, Serenitatis, Crisium, Smythii, and Orientale, also possess regionally low elevations and elevated rims. Another distinguishing feature of the Moon's shape is that the elevations are on average about 1.9 km higher on the far side than the near side. If it is assumed that the crust is in isostatic equilibrium, and that the density of the crust is everywhere the same, then the higher elevations would be associated with a thicker crust. Using gravity, topography and seismic data, the crust is thought to be on average about thick, with the far-side crust being on average thicker than the near side by about 15 km.
Wapowski is a lunar impact crater located on the lunar near side near the southern pole. The crater is located Southwest of craters von Baeyer and Svedberg just inside the rim of the prominent Scott crater. Wapowski was adopted and named after Polish cartographer Bernard Wapowski by the IAU in 2009.
Saussure is a lunar impact crater. It is located in the crater-riddled terrain in the southern hemisphere of the Moon's near side. Just to the north and nearly attached to the rim is the larger crater Orontius. About a half crater diameter due west is the slightly larger crater Pictet.
Capella (below center) and Isidorus (above center). The large crater on the horizon is Theophilus. This shot was taken from the Apollo 11 Lunar Module Eagle. Isidorus is a lunar impact crater that is located to the north of the Mare Nectaris, on the eastern half of the Moon's near side.
Stiborius is a lunar impact crater that lies to the south-southwest of the crater Piccolomini, in the southeastern quadrant of the Moon's near side. To the south-southwest of Stiborius is the smaller Wöhler. Stiborius is 44 kilometers in diameter and 3.7 kilometers deep.Autostar Suite Astronomer Edition. CD-ROM.
Mallet is a crater on the near side of the Moon. It is located next to the linear valley named Vallis Rheita, in the rugged southeastern quadrant. To the northwest along the same valley formation is the crater Young. This is an old formation with a worn and rounded outer rim.
Aristarchus is named after the Greek astronomer Aristarchus of Samos. Like many of the craters on the Moon's near side, it was given its name by Giovanni Riccioli, whose 1651 nomenclature system became standardized in 1935.Ewen A. Whitaker, Mapping and Naming the Moon (Cambridge University Press, 1999), p.61, 210.
Overall, this has caused a trend towards more active but quickly-silenced, closely spaced volcanoes—whereas volcanoes on the near side of the hotspot overlap each other (forming such superstructures as Hawaii island and the ancient Maui Nui), the oldest of the Emperor seamounts are spaced as far as apart.
The opposite bank is close to two rowing clubs and a large canoeing and kayaking club. Weybridge Ait has a recreational rowing club, Weyfarers R.C. The Environment Agency has a control centre and boats on the Lock Island. A nautical shop and boat repair business is on the near side.
Hinshelwood is a lunar impact crater located on the lunar near side near the northern pole. The crater is located in between the large craters Peary and Hermite and just South of the northern pole. The crater was adopted and named after English chemist Sir Cyril Norman Hinshelwood by the IAU in 2009.
Svedberg is a lunar impact crater located on the lunar near side near the southern pole. The crater is located Northeast of Scott crater, adjacent to von Baeyer crater, and South of the prominent crater Demonax. The crater was adopted and named after Swedish chemist Theodor Svedberg by the IAU in 2009.
Justus received the Julia Ellsworth Ford Prize in 1935 and 1936, for Gabby Gaffer's New Shoes and Near-Side-And- Far, respectively. In 1950 she was the recipient of a Boys Club of America Junior Book Award for Luck for Little Lihu. The public library in Monteagle, Tennessee, is named for her.
Riccius is a lunar impact crater that is located in the rugged, southeastern part of the Moon's near side. It was named after Italian astronomers Augustinus Riccius and Matteo Ricci. It lies within one crater diameter southeast of the crater Rabbi Levi. To the east-northeast is Stiborius and due south is Nicolai.
Oblique view from Apollo 17, facing north Swift (above center) and Peirce (center) from Apollo 17. The rays from the left are from Proclus. NASA photo. Swift is a small lunar impact crater that is located in the northwestern part of the Mare Crisium, in the northeast part of the Moon's near side.
Ford & Kenneth is a bus rapid transit station on the METRO A Line in Saint Paul, Minnesota. The station is located at the intersection of Kenneth Street on Ford Parkway. Both station platforms are located near-side of Kenneth Street. The station opened June 11, 2016 with the rest of the A Line.
Accelerator and (transmission) brake pedals were set close together. The hood is of the all-weather type and its door sections are carried in an envelope stored behind the back squab. Large tools are kept in the footrest and there is a specially fitted tool cupboard in the near-side running board.
The cast was still not finalized at this point. At Comiket 58 in 2000, Tsukihime Half Moon Edition was released; 300 copies were sold for 1,000 yen each. This version contained Arcueid and Ciel's "Near Side of the Moon" storylines. The final product of Tsukihime was first released at Comiket in December 2000.
Dunthorne is a small lunar impact crater that is located to the northwest of the small lunar mare called Palus Epidemiarum, in the southwest part of the Moon's near side. It was named after British astronomer Richard Dunthorne. It lies to the southwest of the crater Campanus, east of Vitello. Due south is Ramsden.
The Orange Yeoman prototype built at the RRDE in Malvern lacks the IFF antenna on top, but is otherwise typical of the operational systems. On the right is the transmitter, above it the lens, on the left is the reflector, and on the near side of the lens are the eleven receiver feed horns.
January, 1995. The Man in the Moon is on the near side of the moon, which constantly faces Earth because of its tidally locked orbit. This makes Sir Frederick's crater fairly central, since Mare Serenitatis is so easily viewed. Despite its location, Banting is a very small crater and can be difficult to see.
The impact blasted material into Earth's orbit and then the material accreted and formed the Moon. The Moon's far side has a crust that is thicker than that of the near side. This is thought to be because the Moon fused from two different bodies. This hypothesis, although not perfect, perhaps best explains the evidence.
Mee is a lunar impact crater in the southwestern part of the Moon's near side. Overlying the northwestern rim and intruding one-third the distance across the interior floor is Hainzel, a merged triple-crater formation. To the south is the highly elongated crater Schiller. Mee is 132 kilometers in diameter and 2.7 kilometers deep.
Gravity acceleration at the surface of the Moon in m/s2. Near side on the left, far side on the right. Map from Lunar Gravity Model 2011. A major feature of the Moon's gravitational field is the presence of mascons, which are large positive gravity anomalies associated with some of the giant impact basins.
Albategnius is named after Arab astronomer Al- Battani. Like many of the craters on the Moon's near side, it was given its name by Giovanni Riccioli, whose 1651 nomenclature system has become standardized.Ewen A. Whitaker, Mapping and Naming the Moon (Cambridge University Press, 1999), p.61. Earlier lunar cartographers had given the feature different names.
The shooter has three tries to hit the ball. If the ball is not tapped, the shooter gets a letter. If the ball is released from the near side of the table to the object ball, the shooter gets a letter. If the ball goes in a pocket, the next person in order gets a letter.
Satellite craters Nonius is a lunar impact crater. It is located in the rugged southern highlands on the Moon's near side. It was named after 16th century Portuguese mathematician Pedro Nunes, Latinized as Nonius. The northwestern side and about half the interior floor are overlain by the rim and outer rampart of the walled plain Walther.
Menelaus is named after the ancient Greek astronomer Menelaus of Alexandria. Like many of the craters on the Moon's near side, it was given its name by Giovanni Riccioli, whose 1651 nomenclature system has become standardized.Ewen A. Whitaker, Mapping and Naming the Moon (Cambridge University Press, 1999), p.213. Earlier lunar cartographers had given the feature different names.
That dark, circular lunar mare is located in the east-northeasterly part of the Moon's near side. It was named after the American mathematician Benjamin Peirce. Peirce lies to the north of the craters Yerkes and Picard, and southeast of Macrobius located outside the mare. Just over a crater diameter to the north of Peirce is the smaller Swift.
The 26 runner field split into two groups, with Accidental Agent racing towards the rear of the group on the near side (the left side from the jockeys' viewpoint). He made rapid progress approaching the final furlong, took the lead in the closing stages and kept on strongly to win by a length from the filly Simmie.
Licetus is a lunar impact crater on the near side of the Moon, in the rugged southern highland region. It lies to the south of the walled plain Stöfler, and is attached to the northern rim of the sub-divided crater Heraclitus. Just to the southeast is Cuvier. Licetus is 75 kilometers in diameter and 3.8 kilometers deep.
Forrest Hill. The Sunset Road overbridge and the Upper Harbour Highway interchange northbound offramp can be seen in the background on the far right. The Northern Busway can be seen on the near side of the motorway. The Northern Motorway skirting the edge of the Waitematā Harbour on the northern approach to the Auckland Harbour Bridge.
Reichenbach is a crater in the rugged southeastern part of the Moon's near side. It is located to the west-northwest of the prominent crater Stevinus, and to the west of Snellius. The rugged rim of this crater has been heavily worn by impact erosion. The rim is wider along the northern side, and has a slightly distorted appearance.
The third is collecting lunar samples from the near-side and sending them to Earth, a task for the future Chang'e 5 and Chang'e 6 missions. The fourth phase consists of development of a robotic research station near the Moon's south pole.China's Planning for Deep Space Exploration and Lunar Exploration before 2030. (PDF) XU Lin, ZOU Yongliao, JIA Yingzhuo.
The third is collecting lunar samples from the near-side and sending them to Earth, a task for the future Chang'e 5 and Chang'e 6 missions. The fourth phase consists of development of a robotic research station near the Moon's south pole.China's Planning for Deep Space Exploration and Lunar Exploration before 2030. (PDF) XU Lin, ZOU Yongliao, JIA Yingzhuo.
The third is collecting lunar samples from the near-side and sending them to Earth, a task for the future Chang'e 5 and Chang'e 6 missions. The fourth phase consists of development of a robotic research station near the Moon's south pole.China's Planning for Deep Space Exploration and Lunar Exploration before 2030. (PDF) XU Lin, ZOU Yongliao, JIA Yingzhuo.
Mare Orientale (Latin orientāle, the "eastern sea") is a lunar mare. It is located on the western border of the near side and far side of the Moon, and is difficult to see from an Earthbound perspective. Images from spacecraft have revealed it to be one of the most striking large scale lunar features, resembling a target ring bullseye.
With the piccolo, it becomes necessary to place the near side of the embouchure hole slightly higher on the lower lip, i.e. above the lip margin, and greater muscle tone from the lip muscles is needed to keep the stream/pressure of air directed across the smaller embouchure hole, particularly when playing in higher piccolo registers.
In the semifinals, Wake Forest hosted the three-seed, Louisville. Wake Forest struck first in the match, with Hayden Partain netting the opening goal of the contest in the 29th minute. Louisville's Tim Kübel scored on the near side of the Wake Forest defense with 50 seconds remaining in regulation, in order to force sudden death overtime.
As the horses were walking along Walton Lane the lorry approached and went past them. West Tip was the last in the string and whipped round as the lorry went by. Unfortunately a hook on the bed of the lorry caught West Tip on his near side hindquarters and tore a huge hole. The lorry did not stop.
Centred south-east is junction 11 of the M25 London Orbital Motorway. Circuitously the north of the village is connected, in scenic road skirting St Ann's Hill to Chertsey; the south is more directly connected to the Woking-Staines road. Chertsey railway station is on the near side of the town, from the centre of Lyne.
The third is collecting lunar samples from the near-side and sending them to Earth, a task for the future Chang'e 5 and Chang'e 6 missions. The fourth phase consists of development of a robotic research station near the Moon's south pole.China's Planning for Deep Space Exploration and Lunar Exploration before 2030. (PDF) XU Lin, ZOU Yongliao, JIA Yingzhuo.
The third is collecting lunar samples from the near-side and sending them to Earth, a task for the future Chang'e 5 and Chang'e 6 missions. The fourth phase consists of development of a robotic research station near the Moon's south pole.China's Planning for Deep Space Exploration and Lunar Exploration before 2030. (PDF) XU Lin, ZOU Yongliao, JIA Yingzhuo.
LRO; Promontorium Laplace is labeled at upper-right. Helicon crater (left), with Promontorium Laplace on horizon, from Apollo 15. Promontorium Laplace is a raised mountainous cape situated at the end of Montes Jura in Mare Imbrium on the near side of the Moon. Its selenographic coordinates are 46.8° N, 25.5° W and it is 2600 meters high.
All manned and unmanned soft landings had taken place on the near side of the Moon, until 3 January 2019 when the Chang'e 4 spacecraft made the first landing on the far side. Astronomers have suggested installing a large radio telescope on the far side, where the Moon would shield it from possible radio interference from Earth.
The moon rabbit or moon hare is a mythical figure who lives on the Moon in Far Eastern folklore, based on pareidolia interpretations that identify the dark markings on the near side of the Moon as a rabbit or hare. The folklore originated in China and then spread to other Asian cultures.Windling, Terri. The Symbolism of Rabbits and Hares.
Triesnecker is a prominent lunar impact crater that is located in the Sinus Medii, near the central part of the Moon's near side. Its diameter is 25 km. It was named after Austrian astronomer Franz de Paula Triesnecker. It is located to the north-northwest of the crater Rhaeticus, and to the east- southeast of the flooded Murchison.
Littrow is a lunar impact crater that is located in the northeastern part of the Moon's near side, on the east edge of Mare Serenitatis. Its diameter is 29 km. The crater is named after Bohemian astronomer Joseph Johann Littrow. Some distance to the northeast is the prominent crater Römer, while to the south is Vitruvius.
Manilius is named after the Roman astronomer Marcus Manilius. Like many of the craters on the Moon's near side, it was given its name by Giovanni Riccioli, whose 1651 nomenclature system has become standardized.Ewen A. Whitaker, Mapping and Naming the Moon (Cambridge University Press, 1999), p.61. Earlier lunar cartographers had given the feature different names.
The far side is often inaccurately called the "dark side", but it is in fact illuminated as often as the near side: once every 29.5 Earth days. During new moon, the near side is dark. The Moon had once rotated at a faster rate, but early in its history its rotation slowed and became tidally locked in this orientation as a result of frictional effects associated with tidal deformations caused by Earth. With time, the energy of rotation of the Moon on its axis was dissipated as heat, until there was no rotation of the Moon relative to Earth. In 2016, planetary scientists using data collected on the much earlier NASA Lunar Prospector mission, found two hydrogen-rich areas (most likely former water ice) on opposite sides of the Moon.
Earth's albedo is three times as high as that of the Moon (due in part to its whitish cloud cover), and coupled with the wider area, the full Earth glows over 50 times brighter than the full Moon at zenith does for the terrestrial observer. This Earth light reflected on the Moon's un-sunlit half is bright enough to be visible from Earth, even to the unaided eye – a phenomenon known as earthshine. As a result of the Moon's synchronous rotation, one side of the Moon (the "near side") is permanently turned towards Earth, and the other side, the "far side", mostly cannot be seen from Earth. This means, conversely, that Earth can be seen only from the near side of the Moon and would always be invisible from the far side.
Labeled photo showing location of several craters, Florey in the center. (Click to enlarge) Florey is a lunar impact crater on the lunar near side near the northern pole. Florey is directly adjacent to Byrd crater (diameter of 94 km) to the Southeast and Peary crater (diameter of 73 km) to the North. The crater is named after Australian scientist Howard Florey.
On hearing the second whistle I rushed up Newcastle-street and met Andrews who shouted out, "Come on, quick." I threw my cape to the ground and rushed up after him. I saw a woman lying on the pavement on the near side with her throat cut, and her head lying in a pool of blood. The legs and stomach were exposed.
The vehicle was a traditional coupe, with the novel third seat extending from the side of the car over the near side running board. Paige advertised the Daytona as being "The most beautiful car in America." Paige also produced less-expensive range of cars between 1923-1926. These were sold as Jewetts and were named for the Paige company president H. M. Jewett.
The last century that not all parts of the near side and the surrounding parts of the far side saw only as partial was the 18th century. On Earth, they are seen as total penumbral eclipses. The Moon passes a narrow path within the penumbra and outside the umbra. It can happen on the Earth's northern or southern penumbral edges.
Cuvier is a lunar impact crater on the southern part of the Moon's near side. It is attached to the east-southeast rim of the unusually shaped formation Heraclitus. To the northeast is the crater Clairaut. The rim of this crater has been worn and eroded by subsequent impacts, leaving an outer wall that has been rounded and diminished in prominence.
Goodacre is a lunar impact crater. It is located in the rugged southern highlands on the Moon's near side, and is attached to the north-northeastern part of the exterior of Gemma Frisius, a heavily worn and much larger formation. About two crater diameters to the north of Goodacre lies Pontanus. The crater is named after British selenographer Walter Goodacre.
Kaiser is a lunar impact crater. It lies in the crater-riddled terrain in the southern part of the Moon's near side. It was named after the Dutch astronomer Frederik Kaiser. The crater is nearly attached to the northeast rim the slightly larger crater Fernelius, and the two are separated by an irregular patch of ground only a few kilometers wide.
Rothmann is an impact crater that is located in the southeastern part of the Moon's near side, about one crater diameter to the southwest of the Rupes Altai scarp. To the southwest is the slightly larger crater Lindenau. This is a relatively fresh crater that is not significantly eroded. The outer rim is circular and is not overlaid by craters of note.
Tycho is named after the Danish astronomer Tycho Brahe. Like many of the craters on the Moon's near side, it was given its name by the Jesuit astronomer Giovanni Riccioli, whose 1651 nomenclature system has become standardized.Riccioli map of the Moon (1651) Earlier lunar cartographers had given the feature different names. Pierre Gassendi named it Umbilicus Lunaris ('the navel of the Moon').
Vega is an eroded lunar impact crater that is located in the southeastern part of the Moon. It lies on the near side and so can be viewed from the Earth. Less than one crater diameter to the east-southeast is the slightly smaller Peirescius. About one and a half crater diameters to the west is the long Vallis Rheita.
Pitiscus is a lunar impact crater that lies in the southern part of the Moon's near side, just to the northwest of the larger crater Hommel. It was named after German mathematician Bartholomaeus Pitiscus. The crater is worn, but still forms a prominent feature upon the surface. The rim is roughly circular, but appears oval from the Earth due to foreshortening.
Location of Bailly crater, with its marking at the bottom Lunar Orbiter 4 image This is the largest crater on the near side of the Moon. In area it is comparable in size to a small mare. It lies north of the crater Le Gentil and east of Hausen. Further west of Bailly are the (unofficially named) Montes Dörfel mountains.
Construction will occur from 2018 to 2020. Boarding islands with short high-level handicapped-accessible sections will be built at 42nd Avenue. Contrary to the original plan, the stops will remain on the near side of the cross street. Early implementation of some project elements, including painted clear zones where the boarding islands will be located, was done in early 2017.
The town of Harmony, California, November 2007 Harmony is one paved street off of SR 1. The main structure is a "U" shaped building, the former creamery, with the open area being a small plaza. On the far side of the structure is the Harmony Pottery Shop. On the near side is the former post office and a lounge for visitors.
Wilkins is a lunar impact crater that lies in the rugged highlands in the southeastern part of the Moon's near side. It is located to the southwest of the crater Pons and the long Rupes Altai scarp. Just to the southeast lies the larger crater Zagut, and to the north-northwest is the still-larger Sacrobosco. Wilkins is 57 kilometers in diameter.
LRO image Promontorium Fresnel (Latin for "Cape Fresnel") is a headland on the near side of the Moon. It is located at the northern end of the Montes Apenninus and separates the lunar mares of Mare Serenitatis and Mare Imbrium. Just west of the mountainous cape is Rimae Fresnel. Both features were named after the French physicist Augustin-Jean Fresnel.
Henry Frères is a lunar impact crater that is located in the southwestern part of the near side of the Moon. It was named after the brothers Paul Henry and Prosper Henry, French astronomers. It lies just to the west-northwest of the crater Henry, a similar diameter feature. To the west-southwest of Henry Frères is the much larger crater Byrgius.
Just as with road outfits, early sidecarcross outfits were little more than a solo bike with a sidecar^ Oxford English Dictionary (2nd ed.). Oxford University Press. 1989. "b. A vehicle designed to be attached to the (near-)side of a motor-cycle to accommodate one or more passengers. Occas. attached to a bicycle." attached to its frame by metal tubes.
Snelling & Dayton is a bus rapid transit station on the METRO A Line in Saint Paul, Minnesota. The station is located at the intersection of Dayton Avenue on Snelling Avenue, just south of Marshall Avenue. Both station platforms are located near-side of Dayton Avenue. The METRO B Line, an upcoming bus rapid transit line, is planned to share existing station infrastructure.
Neander is a lunar impact crater that is located to the south of Mare Nectaris, in the southeastern part of the Moon's near side. It was named after 16th century German mathematician Michael Neander. To the west-northwest lies the prominent crater Piccolomini. The northwestern extension of the Vallis Rheita lunar valley passes about a crater diameter to the west of this formation.
Aerial photo of the Descartes Highlands with features and Apollo 16 mission traverses labeled. The Descartes Highlands is an area of lunar highlands located on the near side that served as the landing site of the American Apollo 16 mission in early 1972. The Descartes Highlands is located in the area surrounding Descartes crater, after which the feature received its name.
The third phase is collecting lunar samples from the near side and sending them to Earth, a task for the future Chang'e 5 and Chang'e 6 missions. The fourth phase consists of development of a robotic research station near the Moon's south pole.China's Planning for Deep Space Exploration and Lunar Exploration before 2030. (PDF) XU Lin, ZOU Yongliao, JIA Yingzhuo.
Rough Habit, a bay gelding with a distinctive white blaze trailing over his near-side nostril, was foaled on 2 December 1986. He was sired by Roughcast (USA) out of Certain Habit (NZ) by Ashabit (GB). Certain Habit was the dam of 11 named foals that were produced in Australia and New Zealand, producing 2 stakes winners in Rough Habit and Citi Habit.
Oblique view facing south from Apollo 16 Magelhaens is just above center in this image taken by the crew of Apollo 8. Magelhaens A is left of center, and Goclenius is in foreground. NASA photo. Magelhaens is a lunar impact crater that lies along the southwestern edge of the Mare Fecunditatis, in the eastern part of the Moon's near side.
Regiomontanus is named after the 15th century German astronomer and mathematician Johannes Müller von Königsberg, known as Regiomontanus. Like many of the craters on the Moon's near side, it was given its name by Giovanni Riccioli, whose 1651 nomenclature system has become standardized.Ewen A. Whitaker, Mapping and Naming the Moon (Cambridge University Press, 1999), p.61. Earlier lunar cartographers had given the feature different names.
Montes Teneriffe is a range on the northern part of the Moon's near side. It was named after Tenerife, one of the Canary Islands.Montes Teneriffe at USGS This range is located in the northern part of the Mare Imbrium, to the southwest of the crater Plato. The Montes Teneriffe lie within a diameter of 112 kilometers, although the peaks only occupy a small part of that region.
Epimenides is a lunar impact crater that is located in the southwestern part of the Moon's near side, just to the east of the oddly shaped crater Hainzel. Just to the north and northeast is Lacus Timoris, a small lunar mare. The crater is 27 kilometers in diameter and 2,000 meters deep. It may be from the Pre-Nectarian period, 4.55 to 3.92 billion years ago.
All crewed and uncrewed soft landings had taken place on the near side of the Moon, until 3 January 2019 when the Chinese Chang'e 4 spacecraft made the first landing on the far side of the Moon. On 22 February 2019, Israeli private space agency SpaceIL launched spacecraft Beresheet on board a Falcon 9 from Cape Canaveral, Florida with the intention of achieving a soft landing.
Firmicus is a lunar impact crater that lies in the eastern part of the Moon's near side, so that from Earth it appears oval in shape due to foreshortening. It is, however, very nearly circular. The crater is located to the west of the Mare Undarum, and northeast of the similar-sized crater Apollonius. To the north of Firmicus are the craters van Albada and Auzout.
Schlüter is a lunar impact crater that is located near the western limb of the Moon's near side. It lies along the northwestern face of the Montes Cordillera mountain range that encircles the Mare Orientale. Nearly attached to the eastern rim is the damaged crater Hartwig. Schlüter has an irregular outer rim that is roughly circular, with small outward bulges to the north and southeast.
Debes is a lunar impact crater that is located to the north of the Mare Crisium, in the eastern part of the Moon's near side. It was named after German cartographer Ernst Debes. It lies just to the northwest of the crater Tralles and the prominent Cleomedes. This crater is joined to the oval-shaped Debes A through a break in the southern rim.
The practical benefits of this are more stable long-term orbits and better fuel efficiency. Additionally, the DGE data is hoped to help researchers learn more about lunar origins and the nature of the lunar core. The DGE identified three new near-side mass concentration regions. The purpose of the Lunar Prospector DGE was to learn about the surface and internal mass distribution of the Moon.
Manzinus is a lunar impact crater that is located in the southern region of the Moon's near side. It lies less than one crater diameter to the south- southwest of the crater Mutus, and to the northwest of Boguslawsky. The latter is a crater with nearly the same dimension and a comparable appearance to Manzinus. The outer rim of Manzinus is worn, eroded, and somewhat irregular.
Oblique view from Apollo 10 Maclaurin is a lunar impact crater that is located in the eastern part of the Moon's near side. It lies just to the southeast of the small Mare Spumans, and to the northeast of the prominent crater Langrenus. To the east-southeast is Gilbert. The rim of this crater is perhaps unusual for the number of lesser craters attached to the exterior.
The last of these cradles is the leg cradle. To prepare for the leg cradle, one should get to a near side cradle position, and start pulling one's arms in together for the grip to be set. Before one sets their grip, throw one's legs in on the sides that the leg corresponds to with the hand. Hook one's feet together and lean forward.
Rakwool was up to his usual antics but this time his huge weight overpowered him. He began his leap much too far from the last fence and landed on the near side of it with his chest, throwing his rider clear. Rakwool turned a complete somersault and it was feared he had broken his back. He jarred his entire body and was partly paralysed for many weeks.
Krusenstern is a lunar impact crater that lies amidst the battered terrain in the southern part of the Moon's near side. Nearly attached to the east- southeast rim is the crater Apianus. Less than one crater diameter to the southwest is the prominent Werner. Krusenstern is intruding into a large circular plain to the north designated Playfair G. Playfair itself lies to the northeast.
LRO image Promontorium Archerusia (; Latin for "Cape Archerusia") is a headland on the near side of the Moon. It separates the lunar mares of Mare Serenitatis and Mare Tranquilitatis. Its coordinates are ., accessed 15 February 2019 Promontorium Archerusia was named by Johannes Hevelius and is a misspelling of Acherusia, a cape on the Black Sea near Heraclea in ancient Bithynia (now Karadeniz Ereğli in Turkey).
Elevation map (yellow is highlands and blue is lowlands) Montes Taurus is a rugged, jumbled mountainous region on the Moon. It is located to the east of the Mare Serenitatis, in the northeastern quadrant of the Moon's near side. Coordinates of their center are , and their extent is about 170 km. Montes Taurus are rather unimpressive and indistinct compared to other named lunar mountain systems.
Fourier is a lunar impact crater that is located in the southwestern part of the Moon's near side, just to the southeast of the crater Vieta. To the northeast is the Mare Humorum. The rim of this crater is roughly circular, but appears oval when viewed from the Earth due to foreshortening. Except to the north-northwest, the outer rim is not heavily eroded.
In both of the Near Side of The Moon routes, Shiki discovers a beautiful woman named Arceuid passing by and, in a fit of madness and lust, murders her. However, she reveals herself as an immortal vampire and promises to spare Shiki if he acts as her shield in her quest to kill a vampire. Shiki and Arcueid together then defeat a vampire named Nrvnqsr Chaos.
Alhazen is a lunar impact crater that lies near the eastern limb of the Moon's near side. Just to the south-southeast is the crater Hansen, and to the west is the Mare Crisium. The rim of Alhazen is nearly circular, but appears highly oblong when viewed from the Earth due to foreshortening. The inner walls and the crater floor are rugged and irregular.
The structure, located on 302 North Park Street, remains a staunchly Orthodox Shul. The projecting structure on the near side is the Mikveh. The white clapboard structure with its pointed arched windows closely resembles the small country churches in the region. Inside the building the Aron Kodesh can be seen on the eastern wall and in the center the Bimah where the Sefer Torah was read.
ALICE records first proton-lead collisions at the LHC The analysis of the data from the p-Pb collisions at the LHC revealed a completely unexpected double-ridge structure with so far unknown origin. The proton–lead (pPb) collisions in 2013, two years after its heavy-ion collisions opened a new chapter in exploration of the properties of the deconfined, chirally symmetrical state of the QGP. A surprising near-side, long-range (elongated in pseudorapidity) correlation, forming a ridge-like structure observed in high- multiplicity pp collisions, was also found in high-multiplicity pPb collisions, but with a much larger amplitude (ALICE and ATLAS find intriguing double ridge in proton-lead collisions CERN Courier, 20 February 2013.). However, the biggest surprise came from the observation that this near-side ridge is accompanied by an essentially symmetrical away-side ridge, opposite in azimuth (CERN Courier March 2013 p6).
Freud is a tiny lunar impact crater that lies on a plateau within the Oceanus Procellarum, in the northwest part of the Moon's near side. It is located a few kilometers to the west of the Vallis Schröteri, a large, sinuous valley that begins to the north of the crater Herodotus, then meanders north, then northwest, and finally southwest, until it reaches the edge of the lunar mare.
These new cars offered multiple advantages to the company, as they were lighter, weighing around , seated 36 people, and could be operated by one man. The near-side cars were in length and rode on a single truck.Making a Small Company Pay, p. 908. The benefits of the new cars allowed the company to scrap most of the older cars soon after the arrival of the new replacements.
Oblique view of interior from Apollo 16 Pomortsev is a small lunar impact crater that is located in the eastern part of the Moon's near side. It was named after Russian rocketry scientist Mikhail Pomortsev. It lies on the eastern edge of Mare Spumans, to the southwest of the crater Dubyago. This formation was previously designated Dubyago P. One crater diameter to the north is the smaller Stewart.
NGC 4274 is characterised by its overlapping outer arms, forming a ring structure with apparent diametre 2′.8. The inner arms begin near the edge of the bulge and they are bright and dusty, with dust lanes that more prominent at the near side. Outside the near-ring a set of fainter outer arms has been detected. These outer arms also form a ring, with diametre 5′.9.
Wilson is a lunar impact crater that lies in the southern part of the Moon's near side, to the southwest of the large walled plain Clavius. It is nearly attached to the southeastern rim of the slightly larger crater Kircher. Almost due east lies Klaproth, another walled plain. This crater has a heavily eroded outer rim that now forms an irregular rise about the relatively level interior floor.
Reimarus is a lunar impact crater, located in the southeastern part of the Moon's near side. The eroded southeastern end of the long Vallis Rheita (Rheita valley) passes just to the west. To the northeast is the larger and heavily worn crater Vega. This is a heavily worn and eroded crater, with an outer rim that has been incised and battered by multiple lesser, later impacts, particularly in the western half.
The Reverse Layup is a more stylish method of making the ball from close. Generally, you fake the defender into defending a regular layup on the near side and then jump to the far side of the basket before shooting. One notable Reverse Layup was that of Michael Jordan. His Reverse Layup consisted of him staying on the same side of the hoop while doing the Reverse Layup.
Robinson is a small lunar impact crater that lies to the southwest of the large walled plain J. Herschel. It is located in the continental terrain to the north of the Mare Frigoris, in the northwestern part of the Moon's near side. To the southwest is another walled plain, South. This crater has only been slightly worn through impact erosion, and it retains a sharp outer rim and well-defined features.
LRO image of Nasireddin (lower center), overlapping Huggins crater (lower left,) and bordering Miller crater (upper right). Nasireddin is a lunar impact crater that lies in the rugged terrain in the southern part of the Moon's near side. This crater overlaps two older formations, intruding into the crater Miller to the north and Huggins to the west. To the east of Nasireddin is the much larger walled plain Stöfler.
Another Lunar Orbiter 4 image Cysatus is a lunar impact crater that is located in the southern part of the Moon's near side. It is joined to the northeastern rim of the larger crater Gruemberger, and intrudes slightly into the interior of that formation. Due south is the larger Moretus, and to the east is Curtius. These craters appear foreshortened when observed from Earth because of their far south location.
Church and 27th Street is a station on the San Francisco Municipal Railway light rail network's J Church line. is a light rail stop on the Muni Metro J Church line, located in the Noe Valley neighborhood of San Francisco, California. The station opened with the line on August 11, 1917. The stop has no platforms; passengers wait on the sidewalk on the near side of the intersection.
Ulloa and Forest Side is a light rail stop on the Muni Metro L Taraval line, located at the intersection of Ulloa street and Forest Side Avenue in the West Portal neighborhood of San Francisco, California. The stop opened with the first section of the L Taraval line on April 12, 1919. The stop does not have platforms; passengers wait on the sidewalk on the near side of the intersection.
The final significant takeover was that of Stark's Motor Service of Dunbar in 1964. Stark's had operated some of its services jointly with Scottish Omnibuses for some years, and a proportion of its fleet was already painted in SMT livery. Leyland Fleetline DD65 (OSG 65V), pictured when new at the foot of North Bridge, Edinburgh, in September 1979. It features the recently introduced 'saltire' logo on its near-side cream band.
Donna is a tiny lunar crater on the near side of the Moon. Its name is an Italian female given name, and does not refer to a specific person. It is located in the eastern half of the Mare Tranquillitatis, at the summit of the lunar dome Omega (ω) Cauchy. As such domes are thought to be volcanic in nature, it appears likely that this crater was created by an eruption.
Lev is a tiny lunar crater located in the southeast part of the Mare Crisium in the east of the lunar near side. The crater is located between the larger crater Fahrenheit to the northwest and the wrinkle ridge Dorsa Harker to the southeast. The name Lev does not refer to a specific person; it is a Russian male given name. Northwest of the crater was the Luna 24 landing site.
Lepaute is a small lunar impact crater that is located along the western edge of the Palus Epidemiarum, a minor lunar mare in the southwestern part of the Moon's near side. It was named after French astronomer Nicole-Reine Lepaute. To the east is the larger crater Ramsden, within a system of rilles named the Rimae Ramsden. This is an elongated crater feature that is longer in the north–south direction.
Gentlemen's Doubles final at the 1897 Wimbledon Championships. Players shown are, at the near side, Reginald Doherty (left) and Laurence Doherty (right) and at the far side Herbert Baddeley (left) and Wilfred Baddeley (right). The 1897 Wimbledon Championships was a tennis tournament that took place on the outdoor grass courts at the All England Lawn Tennis Club in Wimbledon, London, United Kingdom. The tournament ran from 21 June until 1 July.
Hagecius is a lunar impact crater in the southeastern part of the Moon's near side. It was named after 16th century Czech naturalist Tadeáš Hájek (Latinized as Thaddaeus Hagecius). This crater forms a triangular formation with the craters Rosenberger to the north-northwest and Nearch to the west-northwest. Like both of these craters, Hagecius has undergone erosion from subsequent impacts, and its outer rim is worn and irregular.
Young, Mattingly and Duke were officially named as the crew of Apollo 16, the fifth lunar landing mission, on March 3, 1971. The Descartes Highlands were chosen as the landing site on June 3, 1971. This was the highest region on the near side of the Moon. It was believed to be volcanic in origin and mainly composed of basalt, based upon the tones of gray observed from Earth.
Oblique Lunar Orbiter 4 image Oblique Apollo 16 image Cannon is a lunar impact crater that is located near the east-northeastern limb of the Moon's near side. It lies just to the northwest of the Mare Marginis, and south-southeast of the crater Plutarch. Farther to the east-northeast is Hubble. This is a worn and eroded formation with an interior floor that has been resurfaced by lava.
Mare Smythii (Latin for "Smyth's Sea") is a lunar mare located along the equator on the easternmost edge of the Moon's near side. It is named for the 19th-century British astronomer William Henry Smyth. The Smythii basin where the mare is located is of the Pre-Nectarian epoch, while the surrounding features are of the Nectarian system. It is contained within a minimal diameter of , and has been excavated to a depth of .
The banking slopes down behind each goal until it reaches the same level as the pitch along the north side. There is hard standing around the entire perimeter of pitch, along with a turnstile block and a gate opening out onto the stadium car park for ambulance access. View of the Walled Meadow's main stand c.1988. Damage sustained during the Great Storm of 1987 can be seen on the near side of the stand.
Other large impact basins such as Imbrium, Serenitatis, Crisium, Smythii, and Orientale also possess regionally low elevations and elevated rims. The far side of the lunar surface is on average about higher than that of the near side. The discovery of fault scarp cliffs by the Lunar Reconnaissance Orbiter suggest that the Moon has shrunk within the past billion years, by about 90 metres (300 ft). Similar shrinkage features exist on Mercury.
Lunar architecture exists both in theory and in practice. Today the archeological artifacts of temporary human outposts lay untouched on the surface of the Moon. Five Apollo Lunar Module descent stages stand upright in various locations across the equatorial region of the Near Side, hinting at the extraterrestrial endeavors of mankind. The leading hypothesis on the origin of the Moon did not gain its current status until after lunar rock samples were analysed.
Clementine image Klaproth is an old lunar impact crater that lies in the rugged southern highlands of the Moon's near side. Due to its location, this crater appears significantly foreshortened when viewed from the Earth. The southern rim of the crater is overlain by the similar-sized crater Casatus, and to the north-northeast lies Blancanus. The outer rim of Klaproth has been deeply eroded, incised, and reshaped by a long history of bombardment.
Condorcet is a lunar impact crater that is located in the eastern part of the Moon's near side, to the southeast of the Mare Crisium. It was named after French mathematician Marquis de Condorcet. To the northeast of Condorcet are the craters Hansen and Alhazen. The outer rim of Condorcet is eroded, with a low saddle point along the northern wall and the satellite crater Condorcet Y lies across the northwestern rim.
The second shot is to play over the mound in front of the green. A roll up and over this mound is punished by a bunker on the left side and is highly undulated. For the first shot a carry of 176 yards from the back of the tee catches the near side of the knoll for a roll over to the level playing ground for the second shot.” - Charles Banks (1925).
Dalton is a lunar impact crater that is located near the western limb of the Moon's near side. It is attached to the eastern rim of the walled plain Einstein, with Balboa lying just to the north and Vasco da Gama due south. The rim of this crater is not heavily eroded, and the interior walls are terraced. The interior floor has a system of rilles that are generally concentric with the inner wall.
240px Shuckburgh is a lunar impact crater that is located in the northeastern part of the Moon's near side, named after George Shuckburgh-Evelyn. It lies south-southeast of the flooded crater Chevallier and northwest of Hooke, roughly midway between these two formations. To the northeast is the Lacus Temporis plain. The interior floor of this crater has been resurfaced with lava, leaving a level plain surrounded by the worn and rounded outer rim.
Rupes Altai in the middle Rupes Altai is an escarpment in the lunar surface that is located in the southeastern quadrant of the Moon's near side. It is named for the Altai Mountains in Asia, and is the most prominent lunar escarpment. The selenographic coordinates of this feature are , and it has a length of about 427 km. The southeastern end of the cliff terminates along the western edge of the crater Piccolomini.
There are many ways to counter the cradle and many variations to the cradle maneuver. For example, there is the "near-side cradle" that is done by a wrestler grabbing the leg of the opponent that is closest to them and then wrapping and locking that with the opponent's neck. There are also a few other cradles. A few examples would be the "far side cradle", the "standing cradle", "clap cradle", and the "leg cradle".
Location of Moigno Moigno is a lunar impact crater that is located in the northern part of the Moon's near side. It lies just to the west of the crater Arnold, and southeast of Neison. The low rim of this crater is worn and eroded, until it is nearly level with the surrounding terrain. The perimeter is only roughly circular, and there are notches along the inner face of the western side.
Lacus Somniorum (Latin somniōrum, "Lake of Dreams") is a plain located in the northeastern part of the Moon's near side. It is located at selenographic coordinates 38.0° N, 29.2° E, and has a diameter of 384 kilometers. (It is the largest of the lunar features designated Lacus.) The name is Latin for Lake of Dreams, a title given to this feature by Riccioli. Lacus Somniorum is an irregular feature with complex, somewhat ill-defined borders.
Fontana is a lunar impact crater that is located in the southwestern part of the Moon's near side, to the south of the Oceanus Procellarum. It lies to the west-northwest of the flooded crater Zupus. Midway between Fontana and Zupus is a rille system designated Rimae Zupus. This is a low-rimmed crater with an interior floor that is marked only by several small craterlets, and a few low ridges in the southwest.
Oblique view facing south from Apollo 15 Another oblique view from Apollo 14 Abel is an ancient lunar impact crater that lies near the southeast limb of the Moon's near side. It is located to the south of the crater Barnard, at the northwest edge of the Mare Australe. The rim of Abel is heavily eroded and distorted in shape, forming a somewhat polygonal figure. It is incised and overlaid by past impacts.
Oceanus Procellarum (Latin Ōceanus procellārum, the "Ocean of Storms") is a vast lunar mare on the western edge of the near side of the Moon. It is the only one of the lunar maria to be called an "Oceanus" (ocean), due to its size: Oceanus Procellarum is the largest of the maria, stretching more than across its north–south axis and covering roughly , accounting for 10.5% of the total lunar surface area.
This crater was named after Ernest Henry Shackleton, an Anglo-Irish explorer of Antarctica from 1901 until his death in 1922. The name was officially adopted by the International Astronomical Union in 1994. Nearby craters of note include Shoemaker, Haworth, de Gerlache, Sverdrup, Slater, and Faustini. Somewhat farther away, on the eastern hemisphere of the lunar near side, are the larger craters Amundsen and Scott, named after two other early explorers of the Antarctic continent.
This near side is variously sunlit, depending on the position of the Moon in its orbit. Thus, the sunlit portion of this face can vary from 0% (at new moon) to 100% (at full moon). The lunar terminator is the boundary between the illuminated and darkened hemispheres. Each of the four "intermediate" lunar phases (see below) is around 7.4 days, but this varies slightly due to the elliptical shape of the Moon's orbit.
Gerard is a lunar impact crater that lies along the western edge of the Oceanus Procellarum near the northwest limb of the Moon's near side. It is located to the north-northwest of the crater von Braun, and northeast of Bunsen. Because of its location, Gerard appears strongly foreshortened when viewed from the Earth, hindering observation. This is a worn and eroded formation with a rim that has been nearly obliterated in some locations and distorted in others.
Thorium concentrations on the Moon. The large area of high concentration on the Near Side (left) corresponds to the Procellarum KREEP Terrane, and the smaller area on the Far Side (right) to the South Pole–Aitken Terrane. The large purple area to the north of this includes the Felspathic Highlands Terrane, which is not reflected in thorium concentrations. The Moon is composed of two major geologic provinces that have a unique origin, composition, and thermal evolution.
Gauricus is a lunar impact crater that is located in the rugged southern part of the Moon's near side. It was named after Italian astronomer Luca Gaurico. Nearly attached to the western rim is the heavily eroded crater Wurzelbauer, and to the north-northwest lies Pitatus. The rim of this crater has become worn and eroded by subsequent impacts, resulting in a round-shouldered outer wall that is pock-marked by a number of lesser craters.
Young is a lunar impact crater that is located in the rugged southeast part of the Moon's near side. It lies to the east of the crater Metius, and southeast of Rheita. The long Vallis Rheita follows a line tangential to the southwest rim of Rheita, and cuts a wide trough through the southwest floor and outer rim of Young. The surviving part of the crater is a worn, eroded formation that has seen better times.
Hell is a lunar crater in the south of the Moon's near side, within the western half of the enormous walled plain Deslandres. To the southeast, also within Deslandres, is the larger crater Lexell, and about 9° to the south lies the prominent Tycho crater. The crater received its name in 1935 after the Hungarian astronomer and ordained Jesuit priest Maximilian Hell. It has 19 satellite craters with diameters ranging between about 3 and 22 km.
Much of the wilderness has given way to settled lands, with plowed fields and lawns visible. Various activities go on in the background: plowing, boat-building, herding sheep, dancing; in the foreground, an old man sketches what may be a geometrical problem with a stick. On a bluff on the near side of the river, a megalithic temple has been built, and smoke (presumably from sacrifices) arises from it. The images reflect an idealized, pre-urban ancient Greece.
At the edges of the near side and a small surrounding part of the hard side where the Earth is mostly half- or partly-seen, in the west, some solar eclipses begin at sunrise, and the Sun is seen after sunrise. In some eclipses, the Sun is partially visible, partially eclipsed in others. In the east, some solar eclipses end at sunset, and the Sun is seen before sunset. In other eclipses, the Sun is partially visible.
Engine near-side Engine off-side Although the Bentley 4½ Litre was heavy, weighing , and spacious, with a length of and a wheelbase of , it remained well-balanced and steered nimbly. The manual transmission, however, required skill, as its four gears were unsynchronised. The robustness of the 4½ Litre's lattice chassis, made of steel and reinforced with ties, was needed to support the heavy cast iron inline-four engine. The engine was "resolutely modern" for the time.
LRO mosaic Chevallier is a lunar impact crater that is located in the northeastern part of the Moon's near side, about a crater diameter east- southeast of the prominent crater Atlas. To the south-southeast of Chevallier is the flooded crater Shuckburgh. This formation is little more than a disintegrated crater rim protruding upward slightly from a lava-flooded surface. All that survives of this feature is a few arcing sections of low ridges in the surface.
G. Bond is a small lunar impact crater to the south of the Lacus Somniorum, a small lunar mare in the northeast part of the Moon's near side. It was named after the American astronomer George Phillips Bond. It lies to the east of the larger crater Posidonius, and to the south of the flooded crater remnant Hall. The crater is situated in a rugged section of terrain to the northwest of the Montes Taurus mountain region.
Maupertuis is the remnant of a lunar impact crater that is located in the northern part of the Moon's near side. It lies in the stretch of rugged terrain north of Sinus Iridum, a bay in the northwestern corner of Mare Imbrium. To the north lies the crater La Condamine, and Mare Frigoris. This is a crater that has been nearly obliterated by a history of impacts, leaving only a disintegrated remnant of the original rim.
Vallis Rheita and Vallis Snellius (detail of LRO map) Vallis Rheita is a linear valley on the near side of the Moon. It is located in the southeastern quadrant, and is oriented radially to Mare Nectaris. This valley appears to share a common origin with the Vallis Snellius to the northeast, as both are oriented radially with Mare Nectaris. The center of the valley lies at selenographic coordinates , and it has a length of 445 km.
At its maximum extent this valley has a width of about 30 km, but it narrows to 10 km at the southeastern extreme. It is the second longest such valley on the near side of the Moon, being exceeded only by Vallis Snellius. Vallis Rheita has been eroded by a series of impacts, and several notable craters lie along the length of this valley. Near the northwestern end is the crater Rheita, for which this formation was named.
Damoiseau is a lunar impact crater that is located just to the west of the Oceanus Procellarum, in the western part of the Moon's near side. It lies due east of the prominent crater Grimaldi, a walled plain with a distinctive dark floor. Due south of Damoiseau is the crater Sirsalis. The low outer rim of Damoiseau is not quite circular, having an outward protrusion to the northeast and smaller bulges to the north and southeast.
Earth-based view of Clavius (North up) Lunar Orbiter 4 view of Clavius Clavius is one of the largest crater formations on the Moon, and it is the second largest crater on the visible near side (very close in size to Deslandres). It is located in the rugged southern highlands of the Moon, to the south of the prominent ray crater Tycho. The crater is named for the Jesuit priest Christopher Clavius, a 16th-century German mathematician and astronomer.
Walther is named after the German astronomer Bernhard Walther. Like many of the craters on the Moon's near side, it was named (in the Latin form, 'Valtherus') by Giovanni Riccioli, whose 1651 nomenclature system has become standardized. Earlier lunar cartographers had given the feature different names: Michael van Langren's 1645 map calls it "Caroli I Reg. Britt.", after King Charles I of England, and Johannes Hevelius grouped it with Purbach and Regiomontanus as "Mons Libanus" after Mount Lebanon.
Oblique view of Schubert and vicinity, facing west, from Apollo 15 Schubert is a lunar impact crater that lies near the eastern limb of the Moon's near side. The crater is located to the northwest of the Mare Smythii, and southwest of the prominent crater Neper. Nearly attached to the southern rim is the crater Back. Schubert is a nearly circular crater formation that has not suffered significant erosion from subsequent impacts, and retains a well-defined rim.
Mons Penck is a mountain promontory on the near side of the Moon. It lies just to the northeast of the crater Kant, to the north of Ibn-Rushd and the Rupes Altai scarp. Southeast of Mons Penck are the prominent craters Theophilus and Cyrillus. The selenographic coordinates of this peak are 10.0° S, 21.6° E. It has a diameter of about 30 km at the base and climbs to an altitude of over 4 km (13,000 feet).
Lunar Orbiter 4 image from 1967 Palus Epidemiarum (Latin palūs epidēmiārum Marsh of Epidemics) is a small lunar mare in the southwestern part of the Moon's near side. This feature forms a rough band of lava-flooded terrain that runs generally west–east, with a northward extension near the western end. It spans a shallow trough extending 300 by 120 km. The average thickness of the basalt is 200–250 m, with a maximum depth of 750 m.
Negotiating the Treaty of Portsmouth (1905). From left to right: the Russians at far side of table are Korostovetz, Nabokov, Witte, Rosen, Plancon; and the Japanese at near side of table are Adachi, Ochiai, Komura, Takahira, Satō. The large conference table is today preserved at the Museum Meiji Mura in Inuyama, Aichi Prefecture, Japan. The Wentworth was built in 1874 by Daniel Chase, a distiller from Somerville, Massachusetts, and for the first two years was named Wentworth Hall.
Location of Apollonius on the near side of the Moon Oblique view from Apollo 10 Oblique view from Apollo 17 Apollonius is a lunar impact crater located near the eastern limb of the Moon. It lies in the region of uplands to the west of Mare Undarum and northeast of the Sinus Successus on the Mare Fecunditatis. It was named after Greek mathematician Apollonius of Perga. It is southwest of the crater Firmicus, and north of Condon.
Baco is a lunar impact crater that lies in the rugged southern highlands on the near side of the Moon. The rim and inner wall has been eroded and worn by countless minor impacts since the original formation of the crater. As a result, any terraces have been worn smooth and the rim is overlaid by several tiny craterlets. The interior floor is nearly flat, with no characteristic central peak at the midpoint and no small craters of significance.
On the east side of the house a serpentine lake was created on the near side of the River Dee. By the 1820s formal garden beds were becoming fashionable and William Andrews Nesfield was employed to design formal parterres around the house. He added more terracing, balustraded walls, and flower beds surrounded by box edging. Grosvenor House, showing the new entrance For the London estate, Grosvenor created a "fashionable new residential quarter" near Buckingham House (later Buckingham Palace).
Rosen, Plancon; and the Japanese at near side of table are Adachi, Ochiai, Komura, Takahira, Satō. The large conference table is today preserved at the Museum Meiji Mura in Inuyama, Aichi Prefecture, Japan. Witte was brought back into the governmental decision-making process to help deal with growing civil unrest. Confronted with increasing opposition and, after consulting with Witte and Prince Sviatopolk-Mirsky, the Tsar issued a reform ukase on December 25, 1904 with vague promises.
These routes are unlocked after completing at least one of the Near-side routes and having low affection with the two previous heroines. This side's stories consist of events pertaining to the Tohno family and its dark history. In all of the Far-Side Routes, Shiki finds that his classmate, Satsuki Yumizuka—who has a crush on him, has disappeared. Seeking to find her, he ignores the blonde haired woman (Arcueid) who passes him by, never encountering her.
A cradle is a move where the attacker performs the cradle by grabbing the neck of his opponent with one arm, and wrapping the elbow of the other arm behind the knee of the opponent. The wrestler then locks both hands together, forcing the opponent's knee toward his face, and rolls the opponent over onto his back. The hooked leg can be either the near leg (a "near-side cradle") or the far leg (a "far-side cradle").
Oblique Lunar Orbiter 5 image, facing west Leibnitz is a huge lunar impact crater that is located in the southern hemisphere on the far side of the Moon. This formation is the same size as Clavius on the near side. It is located to the east-southeast of Mare Ingenii, and is joined to the northeast rim of Von Kármán. Attached to the eastern rim of Leibnitz is Davisson, and intruding into the southeast rim is Finsen.
The Cispadane Republic () was a short-lived republic located in northern Italy, founded in 1796 with the protection of the French army, led by Napoleon Bonaparte. In the following year, it was merged with the Transpadane Republic (formerly the Duchy of Milan until 1796) to form the Cisalpine Republic. These were French client states organized by Napoleon after the Battle of Lodi in May 1796. The republic's name refers to the "near side" of the River Po.
The two hemispheres have distinctly different appearances, with the near side covered in multiple, large maria (Latin for 'seas'). These lowlands were believed to be seas of lunar water by the astronomers who first mapped them, in the 17th century (notably, Giovanni Battista Riccioli and Francesco Maria Grimaldi). Although no bodies of liquid exist on the Moon, the term "mare" (plural: maria) is still used. The far side has a battered, densely cratered appearance with few maria.
Aerial approach to the former base on Johnston Island (top). The ship channel is visible as a darker blue area starting at left and continuing up around the right side of Johnston Island, with Sand Island on the near side (bottom). In 1935, personnel from the US Navy's Patrol Wing Two carried out some minor construction to develop the atoll for seaplane operation. In 1936, the Navy began the first of many changes to enlarge the atoll's land area.
Oblique view from Lunar Orbiter 4 Goldschmidt is a large lunar impact crater of the variety commonly termed a walled plain. It lies in the northern part of the Moon's near side, and appears oval in shape due to foreshortening. The rim is actually relatively circular, although the western rim is overlain by the prominent crater Anaxagoras. Nearly attached to the southeast rim is Barrow, and the two formations are separated by a rugged rise about 30 kilometers across.
Elger is a lunar impact crater that lies along the southern edge of Palus Epidemiarum, the Marsh of Epidemics, in the southwest part of the Moon's near side. To the northeast is the flooded crater Capuanus, and farther to the northwest is Ramsden. The crater is named after British astronomer Thomas Gwyn Elger. The rim of this formation is rough and somewhat eroded formation, with a break and an outward bulge along the northern end, while a ridge intrudes into the southern rim.
Promontorium Agassiz (below center) and Promontorium Deville (left of center), from Lunar Orbiter 4 Oblique view showing Promontorium Agassiz (right), Promontorium Deville (left of center), and Mont Blanc (left, highest peak). From Apollo 15. Promontorium Agassiz is a mountainous cape situated on the northeast margin of Mare Imbrium on the near side of the Moon. Its selenographic coordinates are 42.4° N, 1.77° E. It is located south of Promontorium Deville and Mons Blanc, northeast of Mons Piton, and northwest of Cassini crater.
Promontorium Deville (left of center) and Promontorium Agassiz (below center), from Lunar Orbiter 4 Oblique view showing Promontorium Agassiz (right), Promontorium Deville (left of center), and Mont Blanc (left, highest peak). From Apollo 15. Promontorium Deville is a mountainous cape situated on the northeast margin of Mare Imbrium on the near side of the Moon. Its selenographic coordinates are 43.31° N, 1.14° E. It is located north of Promontorium Agassiz, south of Mont Blanc, northeast of Mons Piton, and northwest of Cassini crater.
Apollo 17 image Heinrich is a small lunar impact crater on the Mare Imbrium, a lunar mare in the northwest quadrant of the Moon's near side. It was named after Czechoslovakian astronomer Vladimír Václav Heinrich. It is a circular, bowl-shaped formation very similar to many other craters of comparable size on the Moon. Heinrich lies to the southwest of the prominent crater Timocharis, and was previously designated as Timocharis A before being given its current name by the IAU.
Oblique view of Fra Mauro taken from lunar orbit on the Apollo 12 mission. The Fra Mauro formation (or Fra Mauro Highlands) is a formation on the near side of Earth's Moon that served as the landing site for the American Apollo 14 mission in 1971. It is named after the 80-kilometer-diameter crater Fra Mauro, located within it. The formation, as well as Fra Mauro crater, take their names from a 15th-century Italian monk and mapmaker of the same name.
The finish of the 1884 Derby from the Illustrated London News. Harvester is on the near side At Epsom on 28 May, on a "cold and cheerless day", Harvester started at odds of 100/7 in a field of fifteen. He was regarded as his trainer’s third string behind Queen Adelaide, who started 5/2 favourite and St Medard (6/1). Harvester was held up in the early stages before moving into contention as Borneo led the field into the straight.
In order to achieve his object he had to cross the whole length of the bridge by himself under intense enemy fire, which increased as his objective became apparent to the Germans. Having disconnected the charges on the far side, he re-crossed the bridge and cut the wires on the near side. It was necessary for him to kneel, forming an easy target, whilst he successively cut the wires. He then discovered that there were also charges underneath the bridge.
LRO image with Huggins at left, and Nasireddin at right Huggins is a lunar impact crater that lies in the rugged southern highlands of the Moon's near side. It was named after British astronomer Sir William Huggins in 1935.Huggins, Gazetteer of Planetary Nomenclature, International Astronomical Union (IAU) Working Group for Planetary System Nomenclature (WGPSN) This crater lies across the eastern rim of the larger crater Orontius. The eastern rim of Huggins is laid across in turn by the slightly smaller crater Nasireddin.
Apollo 12 image Apollo 16 image, facing south: Gaudibert in lower right, satellite craters A and B ("ghost craters") above center, and J at left. Gaudibert is a lunar impact crater that lies along the northeast edge of Mare Nectaris in the eastern part of the Moon's near side. Just to the east is the Montes Pyrenaeus mountain chain, and to the northeast beyond the mountains is the crater Gutenberg. Northwest of Gaudibert is the crater pair Isidorus and Capella.
In areas around seven to eight degrees near the far side, a part of the Earth's view is blocked. In some eclipses, this phenomenon begins not long after sunrise in the west and ends not long before sunset in the east. At that location, they are seen at higher altitudes and at most medium altitudes. At the furthermost areas of the far side within the near side, a part of the Earth is seen but only in the highest portions.
This picture is looking at the western end of the field. The T-Hangars are located on the far side of the runway and the FBO is located near the gas pumps on the near side of the runway. (The approach end of runway 28 is not visible.) Smoketown Airport is an airport open to the public, located in Smoketown, east of Lancaster, in Lancaster County, Pennsylvania, USA. The airport is owned by Marlin Horst and managed by Mel Glick.
General Yamashita (center, on the near side of the table) at the surrender ceremony at Camp John Hay on 3 September 1945. Yamashita, along with 50,500 men of the Shobu Group, held out against the American advance in northern Luzon until 15 August 1945. On 3 September 1945, one day after the official Japanese surrender in Tokyo Bay, Yamashita formally surrendered Japanese forces in the Philippines at Camp John Hay's American Residence in the presence of lieutenant-generals Arthur Percival and Jonathan Wainwright.
A horse is best mounted using a mounting block because it is easier for the rider to mount the horse, it puts less strain on the stirrup leathers when mounting and it decreases the chances of the saddle slipping to one side when mounting, thereby reducing the chances of a fall and possible injury to the rider. A horse or pony is mounted from the "near" side, that is the horse's left side.Mounting a horse or pony from a mounting block.
Dale is a small lunar impact crater located in the far eastern part of the Moon's near side, to the south of the Mare Smythii. It lies to the southeast of the larger crater Kastner and northeast of Ansgarius. The crater is located in a part of the lunar surface that is subject to libration, which can hide it from view for periods of time. It is a relatively shallow and insignificant crater formation with a somewhat eroded outer rim.
It is considered the deepest crater on the near side of the Moon. The interior of Newton is a picture in contrasts. The southern end has been covered, possibly by lava flows or ejecta, leaving a relatively flat surface that is marked only by tiny craters and a slight wrinkle ridge down the middle. The northern half is rugged and irregular, with the satellite crater Newton D overlying the north- northeastern rim and extending across nearly half the crater diameter.
Palmieri is a lunar impact crater that lies to the southwest of the Mare Humorum, in the southwestern quadrant of the Moon's near side. It lies due south of the crater Liebig and east-northeast of the larger Fourier. This crater formation has an eroded outer rim that has a gap along the southeastern side and a pair of narrow gaps along the northern rim. The remains of a small, flooded crater form the northern edge of the gap along the southeast.
The near-side flap is commonly cut forward to keep the rider's right leg and foot from touching the horse's left shoulder. The girthing of an English sidesaddle is usually a three-buckle system, with a usual full-length girth and an additional balancing girth. The stirrup of a sidesaddle is much shorter than in a conventional saddle, so that the rider's knee is placed close to the leaping horn, and it buckles midway down the leather rather than close to the tree.
Lyons Press Horseman's Dictionary p. 194 ;side saddle, sidesaddle #A form of riding where a (normally female) rider sits with both legs to the near side of the horse, rather than with legs astride. #A saddle designed for the above style of riding silhouette, outline diagram :A standard set of diagrams of an individual horse showing its identifying features, including markings and the locations of all its hair whorls. May form part of a horse passport, or of registration/pedigree papers, or both.
Church and Clipper is a light rail stop on the Muni Metro J Church line, located in the Noe Valley neighborhood of San Francisco, California. The station opened with the line on August 11, 1917. The stop has no platforms; passengers wait on the sidewalk on the near side of the intersection. In March 2014, Muni released details of the proposed implementation of their Transit Effectiveness Project (later rebranded MuniForward), which included a variety of stop changes for the J Church line.
Right Of Way/Ocean is a light rail stop on the Muni Metro M Ocean View line, located in the Merced Manor neighborhood of San Francisco, California. It opened in 1925 with the first phase of the line. The station is located where the line's private right-of-way crosses Ocean Avenue, with narrow side platforms located on the near side of the grade crossing. The northbound platform is across the tracks from the southbound platform of Right Of Way/Eucalyptus station.
Right Of Way/Eucalyptus is a light rail stop on the Muni Metro M Ocean View line, located in the Merced Manor neighborhood of San Francisco, California. It opened in 1925 with the first phase of the line. The station is located where the line's private right-of-way crosses Eucalyptus Drive, with narrow side platforms located on the near side of the grade crossing. The southbound platform is across the tracks from the northbound platform of Right Of Way/Ocean station.
Luna 1 impactor Impactor spacecraft are designed to hit the near side of the Moon, transmitting photographs back to Earth until their destruction on impact. Luna 1 (January 1959) missed its intended impact with the Moon and became the first spacecraft to escape the Earth-Moon system. Luna 2 (September 1959) mission successfully hit the Moon's surface, becoming the first man-made object to reach the Moon. This was Luna's only impact success out of six tries from September 1958 to September 1959.
Radiolucency around a 12 day old scaphoid fracture that was initially barely visible. CC-BY 3.0 Seven to nine days after fracture, the cells of the periosteum replicate and transform. The periosteal cells proximal to (on the near side of) the fracture gap develop into chondroblasts, which form hyaline cartilage. The periosteal cells distal to (at the far end of) the fracture gap develop into osteoblasts, which form woven bone through bone resorption of calcified cartilage and recruitment of bone cells and osteoclasts.
Alphonsus is named after King Alfonso X of Castile (known as "Alfonso the Wise"), who had an interest in astronomy. Like many of the craters on the Moon's near side, it was given its name by Giovanni Riccioli, whose 1651 nomenclature system has become standardized; Riccioli originally named it "Alphonsus Rex" ('King Alfonso'), but the 'Rex' was later dropped.Ewen A. Whitaker, Mapping and Naming the Moon (Cambridge University Press, 1999), p.210. Earlier lunar cartographers had given the feature different names.
Oblique view from Apollo 15 Sinus Honoris (Latin sinus honōris "Bay of Honour") is located along the western edge of the Mare Tranquillitatis located on the surface of the near side of the moon. The selenographic coordinates of this feature are 11.7° N, 17.9° E. It has a diameter of 112 km. Sinus Honoris has a wide mouth and is bordered by uneven terrain to the north and southwest. Where the bay joins the mare, rille systems extend to the north and south.
Oblique Lunar Orbiter 5 image, facing west d'Alembert is a large lunar impact crater located in the northern hemisphere on the far side of the Moon, to the northeast of the somewhat smaller walled plain Campbell. Astride the southwest rim of d'Alembert is Slipher. To the north is the crater Yamamoto, and to the south-southwest lies Langevin. This walled plain has the same diameter as Clavius on the near side, making it one of the largest such formations on the Moon.
The basin containing Mare Nubium is believed to have been part of the Pre-Nectarian system. The mare material is of the Imbrian and Eratosthenian age.Geologic Map of the Near Side of the Moon, USGS I-703, Don E. Wilhelms and John F. McCauley, 1971 (L&PI; web version) Bullialdus crater, a prominent feature on the west side of the mare, is of Eratosthenian age. Other features within the mare include Pitatus on the southern margin and Guericke bounding the mare to the north.
Oblique view of Mare Undarum (foreground) and Mare Spumans (upper right), facing south, from Apollo 17 Mare Spumans (Latin spūmāns, the "foaming sea") is a lunar mare located just south of Mare Undarum on the lunar near side. It is one of the many elevated lakes contained in the Crisium basin, surrounding Mare Crisium. The surrounding basin material is of the Nectarian epoch, while the mare basalt being of the Upper Imbrian epoch. The crater Petit (formerly ) is located on the western rim of the mare.
The Procellarum KREEP Terrane is a large province on the near side of the Moon that has high abundances of KREEP. KREEP, an acronym built from the letters K (the atomic symbol for potassium), REE (rare-earth elements) and P (for phosphorus), is a geochemical component of some lunar impact breccia and basaltic rocks. The Felspathic Highlands Terrane, in contrast is composed predominantly of ancient anorthositic materials. A third terrane, the South Pole–Aitken Terrane, may simply represent deep crustal materials of the feldspathic highlands terrane.
The rim and inner wall can still be followed across the surface, but it is indented and notched by smaller impacts. The inner floor contains a pair of small, bowl-shaped craters designated Young A and Young B. To the south of Young, the valley is overlain by Young D, a somewhat less eroded feature than Young. The valley continues intermittently to the southeast, spanning a total distance of about 500 kilometers. This is the longest valley on the near side of the Moon.
Most of the interior floor of this crater has been flooded with basaltic lava, leaving a dark, low-albedo surface that is relatively level and flat. It is somewhat unusual for a crater feature on the far side to be flooded with lava, as the crust is generally thicker than on the near side. The crater is located in the outer rim of the South Pole-Aitken basin. The outer rim of Jules Verne is worn and eroded, with several craters lying across the edge.
Carrington is a lunar impact crater that is located just to the northeast of the crater Schumacher, in the northeastern part of the near side of the Moon. It lies in a stretch of rough terrain between two small lunar maria, with Lacus Temporis to the northwest and the smaller Lacus Spei to the east. To the northeast of Carrington is Mercurius. The rim of Carrington is relatively featureless, with a slight protrusion at the northern end giving the formation a tear-drop shape.
Where near-side stops are present, an advance signal can be highly effective in giving the bus a head start, however the bus stop location needs to consider the detection strategy used for the advance signal phase so that the bus is detected only after it is done serving the bus stop. It is preferable to provide a receiving lane on the far side of the intersection to provide an acceleration/merging area, however this is not always a requirement when an advance signal is used.
Postings in Europe as Minister- Resident to Netherlands and Denmark, and as Minister Plenipotentiary at Rome, Vienna and Bern spanned the years before his 1901 return to Washington, D.C. He then continued as Japan's minister in the United States from 1901 through 1905. Witte, Rosen, Plancoff; and the Japanese at near side of table are Adachi, Ochiai, Komura, Takahira, Satō. The large conference table is today preserved at the Museum Meiji Mura in Inuyama, Aichi Prefecture, Japan. Takahira participated in a number of important Japanese-US negotiations.
In addition to the eclipse, 20 March 2015 was also the day of the March equinox (also known as the spring or vernal equinox in the Northern Hemisphere). In addition, six supermoons were expected for 2015. The supermoon on 20 March 2015 was the third of the year; however, it was a new moon (near side facing away from the sun), and only its shadow was visible. At greatest eclipse, the Sun was at its zenith less than 24 kilometers south of the Equator.
Satellite craters of Bianchini Bianchini is a lunar impact crater that lies along the northern Jura Mountains that ring the Sinus Iridum, in the northwestern part of the near side of the Moon. It was named after Italian astronomer Francesco Bianchini. The impact of this crater near the edge of the Jura Mountains deposited some material into the Sinus Iridum floor. The rim of this crater is not significantly worn, although there is a small crater along the inner side of the eastern rim.
As the PFF gained experience, new problems appeared. Many bombers in the Main Force lost their way to the target and either bombed randomly or turned for home. Another problem was that the illuminators would go out before the raid was complete, leaving the following aircraft to bomb on visible fires, if there were any. This led to the problem of "creepback", when the newly arriving bombers would drop their bombs on the near side of the fire so they could turn for home earlier.
Henry is a lunar impact crater that is located to the northwest of the larger crater Cavendish, in the southeastern part of the Moon's near side. It was named after the Scottish-American scientist Joseph Henry. Less than a half diameter to the northwest is similar-sized crater Henry Frères, named for the brothers Paul and Prosper Henry. The outer rim of Henry has undergone some impact erosion, particularly in the south and southeast where it is overlain by a pair of small craters.
Paneth is a lunar impact crater that is located on the far side of the Moon, just beyond the northwestern limb. It lies just to the north-northeast of the crater Smoluchowski, and to the east-southeast of Boole on the near side. The rim of Paneth is worn but not inordinately so; the edge remains well-defined and marked only by small craters along the northwest and southeast. This formation partly overlies a shallower crater Paneth K along the southeast of the rim.
The Last Supper (1493–1496) is a fresco by the Italian Renaissance painter Pietro Perugino, located in the refectory, now museum, of the former Convent of Fuligno located on Via Faenza #42 in Florence, region of Tuscany, Italy.Polo Museale , city of Florence, official site. The fresco depicts Jesus and the Apostles during the Last Supper, with Judas sitting separately on the near side of the table, as is common in depictions of the Last Supper in Christian art. It is considered one of Perugino's best works.
The distance refers to the near side of the floating platform. For the Large Floating Platform, 300 pounds of HBX-1 is placed 20 feet under water and the distances are 110, 80, 65, and 50 feet from the barge with the first shot Fore-and-aft and the other three shots athwart ship. A hammer test can be used to pre-qualify an item and to identify deficiencies but, ultimately, the items to be certified compliant with MIL-S-901D will be tested on a barge.
Map depicting the battlefield, with al-'Udwatul Dunya and al-'Udwatul Quswa, shown to the right.The valley of Badr is surrounded by two large sand dunes to the east, called al-'Udwatud Dunya (the near side of the valley) and al-'Udwatul Quswa (the far side of the valley). The Qur'an speaks of these two in Surah 8, verse 42. The west of the valley was covered by the al-Asfal Mountain (Jabal Al- Asfal) with an opening between it and another hill in the northwest.
After moving back Shiki has trouble adjusting to the old-fashioned lifestyle his sister lives by. As the story progresses the plot diverges depending upon the choices the character makes. Shiki must use his powers to confront supernatural beings such as vampires, that are known as and . The two plot routes that follow Shiki with Arcueid or Ciel are the Near Side of The Moon routes while the three routes that follow Shiki with Akiha, Hisui or Kohaku are the Far Side of The Moon routes.
A possible configuration of South Pole–Aitken basin sample return spacecraft. On the image, it is on the near side of the Moon. Simulations of near vertical impacts show that the bolide ought to have excavated vast amounts of mantle materials from depths as great as 200 km below the surface. However, observations thus far do not favor a mantle composition for this basin and crustal thickness maps seem to indicate the presence of about 10 kilometers of crustal materials beneath this basin's floor.
Thorium-containing minerals occur on all continents. Thorium is several times more abundant in Earth's crust than all isotopes of uranium combined and thorium-232 is several hundred times more abundant than uranium-235. Thorium concentrations near the surface of the earth can be mapped using gamma spectroscopy. The same technique has been used to detect concentrations on the surface of the Moon; the near side has high abundances of relatively thorium-rich KREEP, while the Compton–Belkovich Thorium Anomaly was detected on the far side.
Planck is a large lunar impact crater, approximately 319 kilometers in diameter, that is located in the southern hemisphere of the Moon, on the far side as seen from the Earth. It lies to the west of the walled plain Poincaré, another enormous formation only slightly larger than Planck. Both formations are larger than the walled plain Bailly, the largest crater on the near side. Lying across the southeast rim of Planck is the crater Prandtl, to the northeast is Hildegard, and to the west is Fechner.
Orontius is a lunar impact crater that lies in the heavily cratered southern highlands of the Moon's near side. It was named after 16th century French mathematician Oronce Fine. It is located to the northwest of the prominent ray crater Tycho, and south and east of the large walled plain Deslandres. The eastern part of the crater is overlain by the smaller crater Huggins, which is overlain in turn on its eastern rim by the still smaller Nasireddin, the trio forming a crater chain of diminishing dimensions.
Low-altitude measurements by the Lunar Prospector showed that this patch is actually a magnetic anomaly--the strongest on the near side of the Moon. This magnetic field may be deflecting particles from the solar wind, and thus preventing the underlying surface from growing darker because of space weathering. This is similar to the process causing Reiner Gamma and other bright swirls such as those of Mare Marginis and Mare Ingenii. About 50 kilometers to the north of this crater was the landing site of Apollo 16.
Lunar Reconnaissance Orbiter image Mons Rümker is an isolated volcanic formation that is located in the northwest part of the Moon's near side, at selenographic coordinates 40.8° N, 58.1° W and is the planned landing site of the Chang'e 5 mission. The feature forms a large, elevated mound in the northern part of the Oceanus Procellarum. The mound has a diameter of 70 kilometres, and climbs to a maximum elevation of about 1,100 metres above the surrounding plain. It was named after Karl L. C. Rümker.
Myomegalin is mostly composed of alpha-helix and coiled-coil structures and has domains shared with microtubule-associated proteins. It has several isoforms, at least two of which have been characterised, CM-MMG and EB-MMG. Myomegalin is necessary for the sufficient growth of microtubules from the centrosomes. The CM-MMG isoform binds at the centrosome with γ-tubulin in an AKAP9-dependent manner and on the near side of the Golgi apparatus, while the EB-MMG isoform binds with MAPRE1 at the Golgi apparatus and increases MAPRE1's effects on microtubule growth.
Oblique view of Ibn Battuta from Apollo 16, facing south Ibn Battuta is a small lunar impact crater on the Mare Fecunditatis, a lunar mare in the eastern part of the Moon's near side. It lies to the southwest of the crater Lindbergh, and northeast of the prominent Goclenius. The crater is circular and symmetrical, with a wide interior floor. The sloping inner walls have a slightly higher albedo than the surrounding mare, but the interior floor is the same dark shade as the exterior of the crater.
Regional map showing location of Hornsby in Mare Serenitatis Hornsby is a tiny lunar impact crater in the western part of the Mare Serenitatis, a lunar mare in the northeast quadrant of the Moon's near side. It was named after British astronomer Thomas Hornsby. It is a solitary formation that is located at least 100 kilometers from any significant craters, although the curiously shaped depression Aratus CA lies about 50 km to the west-northwest. To the north- northwest is Linné, a feature notable for its skirt of high-albedo material.
Lunar Orbiter 4 image Harding is a small lunar impact crater that lies in the Sinus Roris, a bay in the northwest part of the Oceanus Procellarum. Because of its location near the northwest limb of the Moon's near side, this crater is viewed at a relatively low angle from the Earth resulting in foreshortening and limiting the amount of detail that can be seen. This is an isolated formation, making it relatively easy to find. The nearest craters of note are Gerard, farther to the west, and von Braun to the west-southwest.
Cosmos' Stefan Dimitrov followed in the 17th minute with a shot of his own toward the left post which Silverbacks goalkeeper Joe Nasco dove to save. Two minutes later Cosmos defender Hunter Freeman took a corner kick from the near side, but it was sent out of the field. Still, New York continued to mount pressure, with Díaz challenging Nasco twice in a one-minute span. Díaz first placed a shot wide in the 21st minute then got under a cross from Carlos Mendes in the 22nd minute that was also sent wide.
The Pre-Nectarian period is defined from the point at which the lunar crust formed, to the time of the Nectaris impact event. Nectaris is a multi-ring impact basin that formed on the near side of the Moon, and its ejecta blanket serves as a useful stratigraphic marker. 30 impact basins from this period are recognized, the oldest of which is the South Pole–Aitken basin. This geological period has been informally subdivided into the Cryptic and Basin Groups 1-9, but these divisions are not used on any geological maps.
The upper part of the crust probably averages about 88% plagioclase (near the lower limit of 90% defined for anorthosite): the lower part of the crust may contain a higher percentage of ferromagnesian minerals such as the pyroxenes and olivine, but even that lower part probably averages about 78% plagioclase. The underlying mantle is denser and olivine-rich. The thickness of the crust ranges between about 20 and 120 km. Crust on the far side of the Moon averages about 12 km thicker than that on the near side.
On the road, the tester advised, the new Morris Minor S.V. exceeded 50 mph. A certain amount of wheel-bounce consumed a lot of power when testing standing-start times. The tappets could have been adjusted more finely, the accelerator needs a steadier spring and there should be a rest pedal beside it. Speed and brake levers were rather distant, top speed was apt to jump out when the load came off, some wheel bounce and movement with such a short wheelbase is acceptable, the foot brakes pulled to the near-side.
The most widely accepted explanation is that the Moon formed from the debris left over after a giant impact between Earth and a hypothetical Mars-sized body called Theia. New research of Moon rocks, although not rejecting the Theia hypothesis, suggests that the Moon may be older than previously thought. The Moon is in synchronous rotation with Earth, and thus always shows the same side to Earth, the near side. Because of libration, slightly more than half (about 59%) of the total lunar surface can be viewed from Earth.
The near side is marked by dark volcanic maria that fill the spaces between the bright ancient crustal highlands and the prominent impact craters. After the Sun, the Moon is the second-brightest celestial object regularly visible in Earth's sky. Its surface is actually dark, although compared to the night sky it appears very bright, with a reflectance just slightly higher than that of worn asphalt. Its gravitational influence produces the ocean tides, body tides, and the slight lengthening of the day. The Moon's average orbital distance is , or 1.28 light-seconds.
High Desert in California, on the morning of the Trifecta: Full moon, Supermoon, Lunar eclipse, January 2018 lunar eclipse The Moon is in synchronous rotation as it orbits Earth; it rotates about its axis in about the same time it takes to orbit Earth. This results in it always keeping nearly the same face turned towards Earth. However, because of the effect of libration, about 59% of the Moon's surface can actually be seen from Earth. The side of the Moon that faces Earth is called the near side, and the opposite the far side.
Morley is a small lunar impact crater that is located in the eastern part of the Moon's near side, to the east of the Mare Fecunditatis. It was formerly a satellite crater of Maclaurin, being designated Maclaurin R, before being given its current name by the IAU in 1979.Morley, Gazetteer of Planetary Nomenclature, International Astronomical Union (IAU) Working Group for Planetary System Nomenclature (WGPSN) Morley lies to the west-southwest of Maclaurin. This is a small, bowl-shaped crater that is similar to many comparable formations across the lunar surface.
C. W. Snyder, Caltech's Other Rocket Project: Personal Recollections, pp. 7-10, Engineering & Science, Spring 1991 The rockets were launched in a shallow dive, since entry into the water at too steep an angle would defeat their ability to shoot forward at the required shallow depth. The rocket remained lethal even after passing through up to 130 feet of water, giving the pilot a target several times the actual size of the submarine. The sweet spot for targeting was considered to be 60 feet in front of the near side of the submarine.
Weak lensing (gravitational shear) by the intervening universe in general also subtly changes the observed large-scale structure. The large-scale structure of the universe also looks different if one only uses redshift to measure distances to galaxies. For example, galaxies behind a galaxy cluster are attracted to it, and so fall towards it, and so are slightly blueshifted (compared to how they would be if there were no cluster) On the near side, things are slightly redshifted. Thus, the environment of the cluster looks somewhat squashed if using redshifts to measure distance.
While the Moon orbits Earth, Earth rotates once in nearly 24 hours, but its position at the sky is only in one position, as it never changes. This is in contrast to some other moons or other satellites orbiting other planets or dwarf planets and a few asteroids, even inside the Solar System. They are, however, very rare in the outer part of the solar system. The last solar eclipse on the Moon was a total eclipse on January 20, 2019, with the entire near side and tiny surroundings of the far side seeing totality.
Instead they pulled along the near side of Éole and America respectively and brought them to close gunnery duels. Rear-Admiral Thomas Pasley of Bellerophon was an early casualty, losing a leg in the opening exchanges. HMS Royal Sovereign, Graves's flagship, was less successful due to a miscalculation of distance that resulted in her pulling up too far from the French line and coming under heavy fire from her opponent Terrible. In the time it took to engage Terrible more closely, Royal Sovereign suffered a severe pounding and Admiral Graves was badly wounded.
The rim is sharp-edged, and the inner wall material has slumped down to lie in a pile around the base. The interior floor is a rugged jumble, with a small central peak and hills to the north and west. Beyond the rim lies rugged terrain to the north and west, while the ground becomes less jumbled to the southeast beyond the edge of the mountain foothills. This formation should not be mistaken for ths similarly named crater Petit, a small feature on the eastern half of the Moon's near side.
Curie is a large lunar impact crater, much of which lies on the far side of the Moon as seen from the Earth. The western rim projects into the near side of the Moon, as defined by the selenographic coordinate system. However the visibility of this formation depends on the effects of libration, so that it can be brought fully into view or completely hidden depending on the orientation of the Moon. When visible, however, it is seen nearly from the side, limiting the amount of detail that can be observed.
Markov is a lunar impact crater that is located in the northwestern part of the moon’s near side, in the Sinus Roris region of the Oceanus Procellarum. It lies to the south of the crater Oenopides, and is connected to the continental region to the north by ridges along the northern rim. The rim of this crater is not appreciably eroded by impacts, and retains a sharp edge at the crest. The perimeter is roughly circular, with some minor outward bulges particularly along the southern and eastern edge.
Construction will occur from 2018 to 2020. Boarding islands are planned to be built at 26th Avenue; contrary to the original plan, the stops will remain on the near side of the cross street. Early implementation of some project elements, including painted clear zones where the outbound boarding island will be located, was done in early 2017. In response to merchants complaining about the loss of parking spaces to allow for boarding islands, the Board agreed to an experimental pilot program on the inbound side at five stops: 26th, 30th, 32nd, 35th, and 40th Avenues.
Construction will occur from 2018 to 2020. Boarding islands are planned to be built at 32nd Avenue; contrary to the original plan, the stops will remain on the near side of the cross street. Early implementation of some project elements, including painted clear zones where the outbound boarding island will be located, was done in early 2017. In response to merchants complaining about the loss of parking spaces to allow for boarding islands, the Board agreed to an experimental pilot program on the inbound side at five stops: 26th, 30th, 32nd, 35th, and 40th Avenues.
Construction will occur from 2018 to 2020. Boarding islands are planned to be built at 40th Avenue; contrary to the original plan, the stops will remain on the near side of the cross street. Early implementation of some project elements, including painted clear zones where the outbound boarding island will be located, was done in early 2017. In response to merchants complaining about the loss of parking spaces to allow for boarding islands, the Board agreed to an experimental pilot program on the inbound side at five stops: 26th, 30th, 32nd, 35th, and 40th Avenues.
The morphological classification of NGC 1566 is SAB(rs)bc, which indicates a spiral galaxy with a weak bar structure around the nucleus (SAB), an incomplete ring around the bar (rs), and showing moderate to loosely wound arms (bc). The spiral arms are strong and symmetrical. The galactic plane is inclined at an angle of to the line of sight to the Earth and the long axis is oriented along a position angle of . The northwest side of the galaxy is more strongly obscured by dust, suggesting it is the near side.
Short is a lunar impact crater that is located in the southern regions of the Moon, on the near side. It lies just to the south of the larger, prominent crater Moretus, and northeast of Newton. This crater lies across an older crater designated Short B. Only the eroded southeastern section of the rim of Short B still survives. There is a cluster of small craters attached to the outer rim within the attached Short B. Short itself is an eroded formation with a somewhat uneven outer rim.
When Columbia came back around to the near side of the Moon again, he was able to report that the problem had been resolved. For the next couple of orbits, he described his time on the back side of the Moon as "relaxing". After Aldrin and Armstrong completed their EVA, Collins slept so he could be rested for the rendezvous. While the flight plan called for Eagle to meet up with Columbia, Collins was prepared for a contingency in which he would fly Columbia down to meet Eagle.
Oblique view from Lunar Orbiter 5 Close up of Schrödinger G, the low-albedo area within Schrödinger, which is interpreted as a volcanic vent, similar to those in Alphonsus on the near side. Schrödinger is a large lunar impact crater of the form traditionally called a walled plain and is named after Erwin Schrödinger. It is located near the south lunar pole on the far side of the Moon, and can only be viewed from orbit. The smaller crater Ganswindt is attached to the southwestern rim of Schrödinger, and intrudes slightly into the inner wall.
The distribution pattern of the Odin appears similar to that of the thinner, more distal parts of Alpes Formation of the Imbrium Basin on the Moon.Wilhelms, D. E., and McCauley J. F., 1971, Geologic map of the near side of the Moon: U.S. Geological Survey Miscellaneous Geologic Investigations Map I-703, scale 1:5,000,000. The Odin, like the Alpes, occurs in broad lobes such as those in Odin Planitia beyond the main basin scarp. Odin also mantles the intercrater plains ancient crater materials out to a distance of 1200 km from the main Caloris scarp.
When Columbia came back around to the near side of the Moon again, he was able to report that the problem had been resolved. For the next couple of orbits, he described his time on the far side of the Moon as "relaxing". After Aldrin and Armstrong completed their EVA, Collins slept so he could be rested for the rendezvous. While the flight plan called for Eagle to meet up with Columbia, Collins was prepared for certain contingencies in which he would fly Columbia down to meet Eagle.
Mare Anguis (Latin anguis, the "serpent sea") is a lunar mare located on the near side of the Moon, about 150 kilometers in diameter. Located within the Crisium basin, Mare Anguis is a part of the Nectarian System, meaning that it was formed during the Nectarian time period. Like most mare, the surface of Mare Anguis is dark, indicating that it has been filled with volcanic basalt. It forms part of a concentric ring to the northeast of the Crisium rim, and it lies at an elevation 800 m above Mare Crisium.
Gravity anomalies (red) bordering the Procellarum region overlaid on a global elevation map. There are several hypotheses about the origin of Oceanus Procellarum and a related asymmetry between the near and far sides of the Moon. One of the most likely is that Procellarum was a result of an ancient giant impact on the near side of the Moon. The size of the impact basin has been estimated to be more than 3,000 kilometers, which would make it one of the three largest craters in the Solar System.
However, some argue that this term should describe the Moon during the period when it is not reflecting direct sunlight toward Earth. The period when no direct sunlight is reflected by the Moon toward Earth lasts from 21 to 26 hours. The term new moon originally referred to the crescent phase on the first night it is visible, one or two days after conjunction. Maritime records from the 19th century distinguish the dark moon (the time when only earthlight illuminates the near side of the Moon) from the new moon and waning moon.
The appearance is analogous to the tail of a comet that faces away from its star, but comets are solid bodies and much smaller in overall size and mass. Globules located far and close to the central star present different characteristics. On the near side of the Helix Nebula, the central dusty globule of each cometary knot appears dark against the background as it absorbs the [O III] 5007 Angstrom light emitted in the nebular envelope. Those on the far side do not obstruct this light source and so do not have this dark appearance.
The motoring correspondent of The Times published his experiences with the smaller engined sports saloon car in August 1937 soon after its announcement. The handsome body he said offers room for five and really comfortable seating. A driver can climb in and out of the car by the near side without too much difficulty. The luggage compartment contained toolboxes which might have been better stowed below at each side of the spare wheel to avoid being obliged to use the door of the boot as a luggage platform.
Fearless Lad was a "big, strong" chestnut horse with a broad white blaze and two long white socks on his near-side legs bred in England by his owner G Soulsby. He was trained throughout his racing career by Dick Peacock at Middleham in North Yorkshire. He was one of the best horses sired by Import, a sprinter who won the Stewards' Cup in 1975 and the Wokingham Stakes in 1976. His other offspring included the steeplechaser Young Hustler who won the RSA Chase and finished third in the Cheltenham Gold Cup.
Shaler is a lunar impact crater that lies on the southeast interior edge of the Montes Cordillera mountain ring that surrounds the immense Mare Orientale formation. It is located near the southwest limb of the Moon on the near side, and so is viewed nearly from on edge from the Earth. Just to the northwest of the crater is the slightly smaller crater Wright. The long, irregular Vallis Bouvard valley begins at the southern rim of Shaler, and winds its way to the south-southeast towards the crater Baade.
The Tohno blood in him gives him the ability to manipulate his blood into solid objects. ;Fabro Rowan (NRVNQSR- pronounced "Nero")The Hebrew form of the Greek form of "Nero Caesar"; per gematria, this has a value of 666, the number of the beast- see SCM Core Text New Testament, Richard Cooke, SCM Press, 2009, p. 310 :One of the 27 dead apostle ancestors, who to achieve his own immortality fused himself with 666 familiars that he can unleash to feed himself. He is the secondary antagonist of the Near-side routes.
A red bicycle and red man are shown at other times; older crossings do not have a red bicycle – bicycles are permitted to cross at any time (if it is safe to do so).Cyclecraft, p199. Unlike the pelican crossing, before the lights for vehicles go back to green, a steady red and amber are displayed, instead of the flashing amber. The pedestrian/cyclist signal lights may be on the near side of the crossing (like a puffin crossing), or on the opposite side of the road (like a pelican crossing).
Sampling these formations was a priority, as the two cover much of the near side of the Moon. Priority was also given to locating and obtaining samples of old highland material that was older than the Imbrium impact in order to give insight to the geologic timeline and composition of the Moon. North Ray and South Ray craters, both prominent features in the immediate landing area, were also prioritized because material from the prominent formations in the area had been naturally excavated there by the impacts that formed them.
The Edicts of Ashoka refers to the area under Kamboja control as being independent of the Mauryan empire in which it was situated. Some sections of the Kambojas crossed the Hindu Kush and planted Kamboja colonies in Paropamisadae and as far as Rajauri. The Mahabharata locates the Kambojas on the near side of the Hindu Kush as neighbors to the Daradas, and the Parama-Kambojas across the Hindu Kush as neighbors to the Rishikas (or Tukharas) of the Ferghana region.Sethna, K. D. (2000) Problems of Ancient India, New Delhi: Aditya Prakashan.
Lunar Orbiter 4 image of the helmet Apollo 16 image, facing south. This is Figure 28-10 of the Apollo 16 Preliminary Science Report, the caption of which is "Distinct color boundaries of highland mass in Oceanus Procellarum" The Helmet is an informal term for a highland mass within southern Oceanus Procellarum on the near side of the Moon, southeast of the crater Herigonius. The astronauts of Apollo 16 used the term to refer to the feature during the mission.Apollo 16 Preliminary Science Report (NASA SP-315), 1972.
Two planned configurations for a return to the Moon, heavy lift (left) and crew (right) NASA has also outlined plans for human missions to the far side of the Moon. All of the Apollo missions have landed on the near side. Unique products may be producible in the nearly limitless extreme vacuum of the lunar surface, and the Moon's remoteness is the ultimate isolation for biologically hazardous experiments. The Moon would become a proving ground also toward the development of In-Situ Resource Utilization, or "living off the land" (i.e.
Oblique view facing south Lorentz is a huge lunar impact crater that lies just beyond the northwest limb of the Moon, in a region that is brought into sight of the Earth during favorable librations. This formation is nearly as large as the Mare Nectaris on the near side of the Moon, although it has not been submerged by lava as have the lunar mare. Sections of the crater floor are, however, relatively level, particularly an arc along the western rim. But this last region is still marked by a number of tiny craterlets.
Labeled aerial photo of the Taurus–Littrow valley (north is at the bottom). Taurus–Littrow is a lunar valley located on the near side at the coordinates . It served as the landing site for the American Apollo 17 mission in December 1972, the last crewed mission to the Moon to date. The valley is located on the southeastern edge of Mare Serenitatis along a ring of mountains formed between 3.8 and 3.9 billion years ago when a large object impacted the Moon, forming the Serenitatis basin and pushing rock outward and upward.
NGC 547 is a prominent radio galaxy, with two large radio jets of Fanaroff-Riley class I with wide-angle tails. The galaxy is identified as 3C 40B (3C 40A is less prominent and is associated with the nearby galaxy NGC 541), and the source extends for 10 arcminutes in the south-north direction. A small, smooth, dark feature has been observed running across the nucleus in images by the Hubble Space Telescope. Its projected size is 0.3 kpc and its shape suggests it is the near side of a small dust disk.
Tsiolkovskiy is one of the most prominent features on the far side of the Moon. It possesses high, terraced inner walls and a well- formed central peak, which rises over 3200 m above the floor of the crater. The floor is unusual for a crater on the far side, as it is covered by the dark-hued mare that is characteristic of the maria found on the near side. The distribution of the mare material is not symmetrical across the floor, but is instead more heavily concentrated to the east and south.
Clementine mosaic, at high sun angle Lacus Temporis (Latin temporis, Lake of Time) is a small lunar mare that is located in the northeastern quadrant of the Moon's near side. The selenographic coordinates of this feature are , and it lies within a diameter of 117 km. This small mare is composed of two large, roughly circular patches of relatively smooth surface, with a pair of small, cup-shaped craters located prominently at their intersection. Both of these regions of basaltic lava covered surface have some smaller side lobes, which are most likely impact features that have become flooded.
The full moon is the lunar phase when the Moon appears fully illuminated from Earth's perspective. This occurs when Earth is located between the Sun and the Moon (more exactly, when the ecliptic longitudes of the Sun and Moon differ by 180°).[P. Kenneth Seidelmann (ed.), "Phases of the Moon", Explanatory Supplement to the Astronomical Almanac: A Revision to the Explanatory Supplement to the Astronomical Ephemeris and the American Ephemeris and Nautical Almanac, (Mill Valley: University Science Books, 1992), p. 478. This means that the lunar hemisphere facing Earth – the near side – is completely sunlit and appears as a circular disk.
Højbro Plads (literally "High Bridge Square") is a rectangular public square located between the adjoining Amagertorv and Slotsholmen Canal in the City Centre of Copenhagen, Denmark. It takes its name from the Højbro Bridge which connects it to the Slotsholmen island on the other side of the canal while Gammel Strand extends along the near side of the canal. The most striking feature of the square is an equestrian statue of Absalon, the warrior-bishop who has traditionally been credited as the founder of Copenhagen. It was inaugurated in 1901 to commemorate the septcentennial of his death.
Gauss is a large lunar impact crater, named after Carl Friedrich Gauss, that is located near the northeastern limb of the Moon's near side. It belongs to a category of lunar formations called a walled plain, meaning that it has a diameter of at least 110 kilometers, with a somewhat sunken floor and little or no central massif. Due to its location, this crater appears considerably foreshortened when viewed from the Earth, and its visibility is affected by libration. To the northeast of Gauss is Riemann, another walled plain that lies even closer to the limb.
Closer to the nucleus can be observed a dusty spiral pattern, with two arms, with the northwest arm being on the near side of the galaxy, and the southeast one to the far side. The ionised gas inflow rate towards the nucleus is estimated to be 0.2 per year. Although NGC 7213 appears undisturbed in visible light, it shows signs of having undergone a collision or merger when viewed at longer wavelengths, with disturbed patterns of ionized hydrogen including a filament of gas around 64,000 light-years long, itself being part of a larger HI tidal tail southwest of the nucleus.
Control of the province, which bordered directly on Italia, gave the Roman state several advantages: control of the land route between Italy and the Iberian peninsula; a territorial buffer against Gallic attacks on Italy; and control of the lucrative trade routes of the Rhône valley between Gaul and the markets of Massalia. It was from the capital of Narbonne that Julius Caesar began his Gallic Wars. The area became a Roman province in 121 BC, originally under the name Gallia Transalpina (Transalpine Gaul). The name distinguished it from Cisalpine Gaul on the near side of the Alps to Rome.
A Jughandle Intersection "Type A" where turning traffic is diverted away from the main intersection to a slip road. A jughandle is a type of ramp or slip road that changes the way traffic turns left at an at-grade intersection (in a country where traffic drives on the right). Instead of a standard left turn being made from the left lane, left-turning traffic uses a ramp on the right side of the road. In a standard forward jughandle or near-side jughandle, the ramp leaves before the intersection, and left-turning traffic turns left off it rather than the through road.
Excellent earth-based image by Frederic Mallmann Lunar Orbiter 4 image (spots at lower right are blemishes on original) Hausen is a large lunar impact crater that lies along the south-southwestern limb of the Moon. The visibility of this crater is significantly affected by libration effects, although even under the best of conditions it is viewed nearly from on edge. It lies along the western edge of the immense walled plain Bailly. To the northeast is the crater Pingré on the near side, and to the north is the Arrhenius just on the far side of the lunar limb.
Vallis Snellius and Vallis Rheita (detail of LRO map) 斯内利厄斯月谷 Vallis Snellius is a linear valley on the near side of the Moon. It is located in the rugged southeastern part of the visible surface, to the south of the Mare Fecunditatis. This feature is radial to the Mare Nectaris basin to the west- northwest, much like Vallis Rheita to the southwest, and the two likely share a common origin. The selenographic coordinates of this feature are , and it has a maximum length of 592 km, making it the longest named valley on the Moon.
Rille on the valley floor, photographic mosaic from Apollo 15 Lunar Orbiter 4 image (north at top) Schroter's Valley, frequently known by the Latinized name Vallis Schröteri, is a sinuous valley or rille on the surface of the near side of the Moon. It is located on a rise of continental ground, sometimes called the Aristarchus plateau, that is surrounded by the Oceanus Procellarum to the south and west and the Mare Imbrium to the northwest. At the southern edge of this rise are the craters Aristarchus and Herodotus. This is the largest sinuous rille on the Moon.
Phil Stooke, a planetary scientist who studied the lunar crash sites of the LM's ascent stages, wrote that the descent stage "crashed at an unknown location", and another source stated that the descent stage "eventually impact(ed) within a few degrees of the equator on the near side". However, Richard Orloff and an official NASA mission summary stated simply that the descent stage entered lunar orbit, remaining silent on the question of whether the stage later impacted the Moon. An amateur astronomy blog begun in early 2020 explored the possibility that the descent stage may still be in lunar orbit, using computer simulation.
For the rest of the two crafts' passes over the near side of the Moon, Mattingly prepared to shift Casper to a circular orbit while Young and Duke prepared Orion for the descent to the lunar surface. At this point, during tests of the CSM's steerable rocket engine in preparation for the burn to modify the craft's orbit, a malfunction occurred in the engine's backup system. According to mission rules, Orion would have then re-docked with Casper, in case Mission Control decided to abort the landing and use the lunar module's engines for the return trip to Earth.
Mare Orientale is difficult to observe from Earth, as it lies at the extreme western edge of the near side. All that can be seen are the rough mountain ranges—the Montes Rook and the Montes Cordillera—and some glimpses of the dark mare material beyond them. However, the Moon's libration means that on rare occasions Mare Orientale is turned slightly more toward the Earth, and becomes a little more discernible. Although various astronomers had observed hints of the mare, it was first fully described by the German astronomer Julius Franz in his 1906 book Der Mond ("The Moon").
The name feeble grind came from Josh Nelson's friend and fellow skateboarder Sean Donnelley. Sean used to call Josh "the feeb" which was short for feeble, because Nelson was so skinny and often had broken limbs and injuries from skateboarding. Many people watched Josh create this unique type of grind on the parking blocks that were mounted in the reservoir at the Del Mar Skate Ranch. thumb ;Smith grind :This maneuver entails the back truck grinding an edge or rail, while the front truck hangs over the near side of the object, leaving the edge of the deck to rub the lip/edge.
IST (09:13 UTC) by a GSLV Mark III M1. The craft reached the Moon's orbit on 20 August 2019 and began orbital positioning manoeuvres for the landing of the Vikram lander. The lander and the rover were scheduled to land on the near side of the Moon, in the south polar region at a latitude of about 70° south on 6 September 2019 and conduct scientific experiments for one lunar day, which approximates to two Earth weeks. A successful soft landing would have made India the fourth country after the Soviet Union, United States and China to do so.
Oblique Lunar Orbiter 4 image Oblique view from Apollo 16, showing Boss in upper left and Vashakidze in lower right Boss is a lunar impact crater that is located along the northeast rim of the Moon's near side. Due to its location, the crater is viewed from the side by observers on the Earth, and its visibility is subject to libration effects. This formation has not been significantly eroded by impacts, and it retains a well-defined outer rim that is not overlain by smaller craters of note. The inner wall is wide and has a terraced surface.
Oblique Lunar Orbiter 4 image with slightly different lighting Baade is a lunar impact crater that is located near the southwest limb of the Moon on the near side, to the southwest of the enormous Mare Orientale impact basin. The area to the east of this crater forms the junction between the 280-km-long Vallis Bouvard to the north and the narrower, 160-km-long Vallis Baade to the south-southeast. Both valleys radiate away from the impact basin to the north. The outer wall of Baade remains sharp-edged, with little appearance of erosion due to subsequent impacts.
Changes that affect Shiki's opinion on the characters and heroines usually change the direction of the story drastically. Some options can lead to (often violent) deaths for Shiki, after which the player can optionally view a comedic section called 'Teach me, Ciel Sensei!',where Ciel educates the player on their decisions and offers hints on how to avoid them on the next playthrough. There are two scenarios: the Near-Side Route (as in "near-moon") which includes Arcueid and Ciel as selectable heroines, and the Far Side Route (as in far-moon) which includes Akiha, Hisui, and Kohaku as selectable heroines.
Breitbart News initially declined to comment, but on January 8 published a story in which it stood by its claims, which had been shown to be false, and refused to admit to any exaggeration. The only correction issued was with regard to the church's age. The follow-up story used a screen capture of different fireworks at the near side of the church, with no scaffolding. Ruhr Nachrichten, the original outlet and the alleged witness cited by Breitbart News, replied to the update, and stated that Breitbart News had not contacted them or the firefighters present to verify their story.
Apollo 15 image Jeans is a lunar impact crater, on the southeastern limb of the Moon, with its majority lying on the far side. A favorable libration can bring the entire crater into view, but even then the details observable from Earth are very limited as the crater is viewed rather "edge-on". Jeans is located nearly midway between the much larger walled plain Lyot on the near side and the crater Chamberlin on the far side. It has a heavily worn and rounded outer rim, and several impacts lie along the southern and southeastern edge and inner wall.
Oblique view from Lunar Orbiter 5, facing west Campbell is a large lunar impact crater that is located in the northern hemisphere on the far side of the Moon. It lies to the southwest of the walled plain D'Alembert, an even larger formation. If Campbell were located on the near side of the Moon as seen from the Earth, it would form one of the largest visible craters, being slightly larger than Schickard. It is bordered by several craters of note, with Wiener to the southwest, Von Neumann just to the south, Ley overlying the southeast rim, and Pawsey to the west.
The Hague University of Applied Sciences (), abbreviated THUAS, is a university of applied sciences with its campuses located in and around The Hague in the Randstad metropolitan region in the west of the Netherlands. The city is the Dutch seat of government and home to many major international legal, security and peace institutions. Since the university was founded in 1987 it has expanded to four campuses in the near-side cities of The Hague, Delft and Zoetermeer. The main campus in The Hague is located behind The Hague Hollands Spoor railway station by the Laakhaven Canal.
The most notable aspect of Fermi is that the large and prominent crater Tsiolkovskiy intrudes into its southeastern rim. Unlike Tsiolkovskiy, however, the interior of Fermi is not covered by dark basaltic lava, and so it is barely distinguishable from the surrounding rugged and battered terrain. If it were located on the near side of the Moon, however, this would be one of the largest visible craters, with a dimension roughly equal to the crater Humboldt, lying several hundred kilometers to the west-southwest. This formation has been significantly eroded and damaged by subsequent impacts, and several notable craters lie across the rim and within the basin.
Stumps, discarded pieces of tree and other evidence of woodcutting is all around,Solum – over 50 cut trees have been counted in the painting and Lippi has signed his name ("FRATER PHILIPPUS P[inxit]" – "Brother Phillip painted this") along the handle of an axe struck into a stump in the bottom left-hand corner.Hartt, 220; Holmes, 180 A small, evidently fast-running, stream runs down the right- hand side of the painting, crossed by a crude bridge of planks. On the other side of this, near the top of the painting there is a small hut-like building. On the near side of the stream a crane or heron preens itself.
LRO mosaic Oblique view of Mare Undarum (foreground) and Mare Spumans (upper right), facing south, from Apollo 17 Mare Undarum (Latin undārum, the "sea of waves") is an uneven lunar mare located just north of Mare Spumans on the lunar near side, between the crater Firmicus and the eastern limb. It is one of the many elevated lakes contained in the Crisium basin, surrounding Mare Crisium. The selenographic coordinates of this mare are 6.8° N, 68.4° E. It has a maximum diameter of 243 km. The surrounding basin material is of the Nectarian epoch, with the mare basalt being of the Upper Imbrian epoch.
The British held craters 3 and 4 and the near lips of 1, 2, A and B craters and by the near lip of Crater C had been regained and connected to Russian Sap. The Germans then retired to the near lips on the German side. It later emerged that the Germans had driven new galleries through the clay layer on top of the chalk, which could be dug quietly, contributing to the surprise of the German mine explosions. The 35th Brigade relieved the 37th Brigade and by the time that the crater fighting died down, both sides held the near side of each crater.
On the throne, the king has the donkey's ears of King Midas, and Ignorance on his far side and Suspicion on the near side grasp these as they speak into them. The king extends his hand towards Calumny, but his eyes look down so that he cannot see the scene.Lightbown, 234 These identifications are clear from Lucian's description of a painting by Apelles, a Greek painter of the Hellenistic Period. Though Apelles' works have not survived, Lucian recorded details of one in his On Calumny: > On the right of it sits Midas with very large ears, extending his hand to > Slander while she is still at some distance from him.
Rabbi Levi is a lunar impact crater that is located among the rugged highlands in the southeastern part of the Moon's near side. Several notable craters are located nearby, including Zagut just to the north-northwest, the heavily impacted Riccius to the southeast, and Lindenau to the northeast next to Zagut. This is a heavily worn and eroded crater formation, with several smaller craters lying along the incised rim and across the interior floor. A group of these craters form a cluster in the western part of the floor, consisting of the satellite craters A, L, M, and D, as well as lesser craterlets trailing away to the south-southeast.
Oblique view facing south from Apollo 8 Oblique view facing south from Apollo 16 Crozier is a lunar impact crater that is located on the southwest edge of Mare Fecunditatis, a lunar mare in the eastern part of the Moon's near side. It lies to the east-northeast of the prominent crater Colombo, and southeast of the small crater Bellot. The narrow rim of this crater forms a distorted enclosure that has outward bulges along the northwest, southwest, and southeastern sides. The interior floor has been resurfaced and nearly filled by basaltic lava, producing a level surface with a low albedo that matches the dark hue of the nearby lunar mare.
Again, date given by Castanheda (p. 208). As the tide was high during the morning, Palignar was impassable to Naubeadarim's infantry, so Pacheco left the bateis with only a small crew under the command of Andrade and Jusarte, and rushed most of his forces on longboats down to Palurte. A contingent of Cochinese Nairs accompanied Pacheco, although the bulk stayed with prince Candagora at the near side of the Palignar ford. The clearing of the vegetation on the opposite banks immediately paid off as, upon reaching Palurte, Pacheco easily noticed a number of Calicut cannons being rolled into position, aiming to sink the anchored caravels.
1914 International Lawn Tennis Challenge (Davis Cup) finals match between Australasia and the United States played at the West Side Tennis Club in New York on 13–15 August. Players shown on the near side are Norman Brookes (left) and Anthony Wilding (right) for Australasia and on the far side Thomas Bundy (left) and Maurice McLoughlin (right) for the United States. The British 1914 Davis Cup team consisting of Herbert Roper Barrett (top left), Algernon Kingscote (top right), James Cecil Parke (bottom left) and Theodore Mavrogordato (bottom right). The 1914 International Lawn Tennis Challenge was the 13th edition of what is now known as the Davis Cup.
The layout of the scene resembles that seen in the Andrea del Castagno's Last Supper frescoed some 3 to 4 decades earlier for the refectory of Sant'Apollonia in Florence, wherein the apostles sit in a shallow U-shaped setting, with only the two flanking apostles sitting at a 90 degree angle with the others. John the Apostle at Christ's left has fallen to sleep. Judas sits apart on the near side of the table, as is common in early depictions of the Last Supper in Christian art. However, in this depiction, the upper register is not interior, but opens up into the tree-line orchard with birds.
Oblique view from Lunar Orbiter 4 Another oblique view from Lunar Orbiter 4 De La Rue is the remnant of a lunar impact crater, or possibly several merged craters, creating a formation sometimes called a walled plain. It lies in the northeastern part of the Moon on the near side, and so appears foreshortened due to its location. This formation lies to the north-northwest of the prominent crater Endymion, just beyond the eastern extreme of Mare Frigoris. The crater Strabo intrudes into the northern part of De La Rue's northern rim, and the smaller Thales is attached to the northwestern part of the wall.
In this graph, the attractive force decreases in proportion to the square of the distance, while the slope relative to value decreases in direct proportion to the distance. This is why the gradient or tidal force at any point is inversely proportional to the cube of the distance. The tidal force corresponds to the difference in Y between two points on the graph, with one point on the near side of the body, and the other point on the far side. The tidal force becomes larger, when the two points are either farther apart, or when they are more to the left on the graph, meaning closer to the attracting body.
Some of its scientific aims are to conduct studies of lunar topography, mineralogy, elemental abundance, the lunar exosphere, and signatures of hydroxyl and water ice. The Vikram lander, carrying the Pragyan rover, was scheduled to land on the near side of the Moon, in a south polar region at a latitude of about 70° south at approximately 1:50 am(IST) on 7 September 2019. However, the lander deviated from its intended trajectory starting from an altitude of 2.1 kilometres (1.3 mi), and telemetry was lost seconds before touchdown was expected. A review board concluded that the crash-landing was caused by a software glitch.
The plaza contains a large collection of vivid and creative art works as the result of many highly respected national and local graffiti artists working at the Buszy, who painted the large, free, legal wall that is situated at the near side of the designated skate area. All of the four basic elements of hip hop: breakdancing, graffiti, MC-ing, and DJing, have local history rooted to the spot. For example, members of the band Hacktivist would come to the skate jams to perform before the group was formed, gaining worldwide fame. Dance crew would regularly be seen practising in front of the reflective windows of the bus station.
Orbital photo of the Hadley-Apennine site; Apollo 15 landing site is marked with a circle. Hadley–Apennine is a region on the near side of Earth's Moon that served as the landing site for the American Apollo 15 mission, the fourth manned landing on the Moon and the first of the "J-missions", in July 1971. The site is located on the eastern edge of Mare Imbrium on a lava plain known as Palus Putredinis. Hadley–Apennine is bordered by the Montes Apenninus (often referred to as "Apennine Front"), a mountain range, and Hadley Rille, a meandering channel, on the east and west, respectively.
Oblique view from Lunar Orbiter 4 Oblique view from Apollo 16 Lacus Spei (Latin speī, "Lake of Hope") is a small lunar mare that is located in the northeastern part of the Moon's near side. To the north is the crater Mercurius and to the west-southwest lies Schumacher. The selenographic coordinates of this feature are 43.0° N, 65.0° E, and it lies within a diameter of 77 km.Lacus Spei, Gazetteer of Planetary Nomenclature, International Astronomical Union (IAU) Working Group for Planetary System Nomenclature (WGPSN) The main part of the lake occupies a region averaging about 50 km in diameter, with an extension leading to the northeast.
Renzo Piano designed the South Exelon Pavilions (the two structures on the near side of the street in Lurie Garden), the Art Institute's 2009 Modern Wing, and the Nichols Bridgeway. The pavilions are named for Exelon, a Chicago-based company that generates the electricity transmitted by its subsidiary Commonwealth Edison (ComEd). The city of Chicago has collaborated with Exelon and ComEd on a variety of environmental projects, including the installation of solar power in buildings, support for sustainable design and renewable energy, and furthering educational and social awareness of green architecture in the city. The pavilions cost $7 million, $5.5 million of which was donated by Exelon and ComEd.
Far side of the Moon, photographed by Apollo 16 The far side of the Moon is the hemisphere of the Moon that always faces away from Earth. The far side's terrain is rugged with a multitude of impact craters and relatively few flat lunar maria compared to the near side. It has one of the largest craters in the Solar System, the South Pole–Aitken basin. Both sides of the Moon experience two weeks of sunlight followed by two weeks of night; even so, the far side is sometimes called the "dark side of the Moon", where "dark" is used to mean unseen rather than lacking sunlight.
In 1944, as a first lieutenant, John S. Thompson led his men during an air raid as part of Operation Market Garden. The light in the jump bay of the platoon's C-47 Skytrain came on later than expected, moving their landing zone from its intended location near Grave, North Brabant; the plane was passing over buildings when the paratroopers were signalled to leave the aircraft, and Thompson decided to wait until reaching several approaching fields.Ryan, p. 239. Thompson led his platoon in an attack against the nearby bridge spanning the Maas River, which was defended by German forces supplemented by two 20 mm flak guns, one on the near side of the bridge and one across the river.
Daedalus on the Moon's far side The other major geologic process that has affected the Moon's surface is impact cratering, with craters formed when asteroids and comets collide with the lunar surface. There are estimated to be roughly 300,000 craters wider than on the Moon's near side alone. The lunar geologic timescale is based on the most prominent impact events, including Nectaris, Imbrium, and Orientale, structures characterized by multiple rings of uplifted material, between hundreds and thousands of kilometers in diameter and associated with a broad apron of ejecta deposits that form a regional stratigraphic horizon. The lack of an atmosphere, weather and recent geological processes mean that many of these craters are well- preserved.
Arcade screenshot Konami's Ping Pong can be played singleplayer or multiplayer, using 11 point scoring rules; the first player to attain a score of 11 or higher, leading by two points, wins the game (to a maximum of 14-14, at which point the next point wins). The player must win the best of two out of three games in order to beat the match. The playfield is shown from an isometric perspective with the players shown as disembodied hands; players placed on the far-side of the table will find hitting the ball is much more difficult. However, the player is always positioned on the near side during the single player mode.
Witte, Rosen, Plancon; and the Japanese at near side of table are Adachi, Ochiai, Komura, Takahira, Satō. The large conference table is today preserved at the Museum Meiji-mura in Inuyama, Aichi Prefecture, Japan. Military leaders and senior tsarist officials agreed before the war that Russia was a much stronger nation and had little to fear from the Oriental newcomer. The fanatical zeal of the Japanese infantrymen astonished the Russians, who were dismayed by the apathy, backwardness, and defeatism of their own soldiers.Donald P. Wright, “‘Clouds Gathering on the Horizon’: The Russian Army and the Preparation of the Imperial Population for War, 1906-1914,” ‘’ Journal of Military History’’ 83#4 (Dec 2019 ) pp 1133 - 1160, quoting p. 1136-37.
These observations were for the purposes of obtaining multi-spectral imaging of the entire lunar surface, assessing the surface mineralogy of the Moon, obtaining altimetry from 60N to 60S latitude, and obtaining gravity data for the near side. There were also plans to image and determine the size, shape, rotational characteristics, surface properties, and cratering statistics of Geographos. Clementine star tracker view of the Moon and Venus in the distance Clementine carried seven distinct experiments on board: a UV/Visible Camera, a Near Infrared Camera, a Long Wavelength Infrared Camera, a High Resolution Camera, two Star Tracker Cameras, a Laser Altimeter, and a Charged Particle Telescope. The S-band transponder was used for communications, tracking, and the gravimetry experiment.
The lunar far side lacks direct communication with Earth, though a communication satellite at the Lagrangian point, or a network of orbiting satellites, could enable communication between the far side of the Moon and Earth. The far side is also a good location for a large radio telescope because it is well shielded from the Earth. Due to the lack of atmosphere, the location is also suitable for an array of optical telescopes, similar to the Very Large Telescope in Chile. Scientists have estimated that the highest concentrations of helium-3 can be found in the maria on the far side, as well as near side areas containing concentrations of the titanium-based mineral ilmenite.
The first known inhabitants of this region were hunter-gatherers and it was later occupied by pastoralists, shepherds living in caves or simple huts. It later came under the control of a Gaulish tribe called Vellavi and at the time of Julius Caesar's Gallic Wars, this area lay on the border of Gallia Narbonensis. The area became a Roman province in 121 BC, originally under the name Gallia Transalpina (Transalpine Gaul). The name distinguished it from Cisalpine Gaul on the near side of the Alps to Rome. In 40 BC, during the Second Triumvirate, Lepidus was given responsibility for Narbonese Gaul (along with Hispania and Africa), while Mark Antony was given the balance of Gaul.
Post chaise with just a pair of horses, a postilion and one footman in Preston Street, Faversham, 200th anniversary of the Battle of Waterloo How Lapenotiere carried the news from Falmouth to London A post-chaise is a fast carriage for traveling post built in the 18th and early 19th centuries. It usually had a closed body on four wheels, sat two to four persons, and was drawn by two or four horses. A postilion rode on the near-side (left, nearest the roadside) horse of a pair or of one of the pairs attached to the post-chaise"Re- enactment of Lapenotiere's Journey," Exeter Memories, 15 August 2009 leaving passengers a clear view of the road ahead.
Daxia River valley within a few km from its fall into the Liujiaxia Reservoir. The near side of the river is in Linxia County, the far side, in Dongxiang Autonomous County Daxia River falling into the Liujiaxia Reservoir The Daxia River () is a tributary of the Yellow River in southern Gansu Province in China's west. The Daxia River starts in eastern Huangnan Tibetan Autonomous Prefecture in Qinghai, then flows easterly through northern Gannan Tibetan Autonomous Prefecture where its drainage basin covers large parts of Hezuo County-level City and Xiahe County. It then flows northeast into Linxia Hui Autonomous Prefecture, where it is crosses the breadth of Linxia County, and Linxia City.
Venus presents a thin crescent in telescopic views as it comes around to the near side between the Earth and the Sun and presents its new phase when it is between the Earth and the Sun. Since the planet has an atmosphere it can be seen at new in a telescope by the halo of light refracted around the planet. The full cycle from new to full to new again takes 584 days (the time it takes Venus to overtake the Earth in its orbit). The planet also changes in apparent size from 9.9 arc seconds at full (superior conjunction) up to a maximum of 68 arc seconds at new (inferior conjunction).
In 358 AD, this practice was accelerated by the wholescale adoption of the entire Salian Franks people into the Empire, providing a ready pool of such recruits. In return for being allowed to settle as foederatii in northern Gallia on the near side of the Rhine, the Franks were expected to defend the Empire's borders in their territory and provide troops to serve in Roman units. In 376, a large band of Goths asked Emperor Valens for permission to settle on the southern bank of the Danube River on terms similar to the Franks. The Goths were also accepted into the empire as foederati; however, they rebelled later that year and defeated the Romans at the Battle of Adrianople.
1928 off side (inlet) 1929 near side (exhaust) White and Poppe Limited owned a Coventry proprietary engine building and gearbox manufacturing business established in 1899. Many early motor vehicle manufacturers making only a small number of vehicles bought in their major components and White and Poppe soon had a large customer base and by 1914 a staff of around 350 people. By then the number of these customers, once as high as 15 or more, had fallen away though not the production volume leaving Dennis Brothers, always an important customer, taking much of their output. Negotiations begun in 1914 culminated in the purchase of White and Poppe by Dennis Brothers in 1919.
In the middle of the nebula, the line splits in two, since one component is redshifted and one is blueshifted. The blueshifted component will appear brighter as it is on the "near side" of the nebula, and is as such subject to a smaller degree of attenuation as the light coming from the far side of the nebula. The tapered edges of the velocity profile stem from the fact that the material at the edge of the nebula is moving perpendicular to the line of sight and so its line of sight velocity will be zero relative to the rest of the nebula. Several effects can contribute to the transverse broadening of the velocity profile.
One of these proposals, a station at Farmdale, was reviewed by the assigned Administrative Law Judge of the CPUC. In her written decision dated 22 March 2010, the judge ruled that the Farmdale Station could be added to the project by including a CPUC-approved Addendum to the Final EIR, without having to redo the entire project's EIR. The final decision to authorize the grade crossing (and thus, construction of Farmdale Station) was made by the commission on 29 July 2010. All trains operating on the Expo line would be required to come to a complete stop at the Farmdale station, which features near-side stations at the intersection of Farmdale Avenue, thus increasing safety for pedestrians and students in the area.
River Walkham at Horrabridge The Walkham is a river whose source is on Dartmoor, Devon, England. It rises in the wide gap between Roos Tor and Great Mis Tor and flows almost due south for approximately leaving the tors and thus National Park behind then south-west for past Woodtown. The river then reaches a village, Horrabridge, with a small compact network of streets mainly on the south or left bank. It receives most of its tributaries which are unnamed headwaters along its south-flowing inception, draining the near side of two series of six tors (peaks) to the west ending in Pew Tor at 320 metres and likewise to the east ending in Leeden Tor at 389 metres (above mean sea level).
The closed cars were refurbished as part of the series of upgrades across the line to include new interior paint, tungsten lamps, and orange and blue exterior paint, a move to make the cars "more attractive to the students" of the University of Virginia, as these were the school's colors. Although the old cars received cosmetic upgrades, the energy inefficiency of the cars, due in part to their heavy weight, caused the railway to seek a new and improved car. Orders were placed with the J.G. Brill Company for five new near-side one-man streetcars sometime around 1913. By June 1914, two additional cars were ordered and placed in service making for a total of seven new streetcars servicing Charlottesville.
Unlike the Earth, which receives the smallest portion being inside the center of the Moon's shadow during total solar eclipses, during total eclipses on the Moon, the center of the Earth's shadow covers the whole near side of the Moon and lasts much longer than on Earth, up to 1.8 hours.Lunar eclipses Some total-partial eclipses have at most half or a part of the Moon being in the center of the Earth's shadow. Unlike the Earth, whose umbral shadow appears black, as the Moon has no atmosphere, the surface appears not just black but red and brown, according to the Danjon scale. This is because the only sunlight available is refracted through the Earth's atmosphere on the edges of the Earth, forming an atmospheric ring.
Instead, the radiation pattern peaks in directions lying in the plane of the loop, because signals received from sources in that plane do not quite cancel owing to the phase difference between the arrival of the wave at the near side and far side of the loop. Increasing that phase difference by increasing the size of the loop has a large impact in increasing the radiation resistance and the resulting antenna efficiency. Another way of looking at a small loop as an antenna is to consider it simply as an inductive coil coupling to the magnetic field in the direction perpendicular to plane of the coil, according to Ampère's law. Then consider a propagating radio wave also perpendicular to that plane.
Oblique photo of Chaplygin from Apollo 11, facing south Oblique photo of a small, young crater Chaplygin B (Chappy) with a bright ray system on the north edge of Chaplygin, from Apollo 11, facing south Oblique photo of Chaplygin from Apollo 13, facing south Highly oblique photo of Chaplygin from Apollo 16, facing south Chaplygin is a large lunar impact crater that lies on the far side of the Moon. It is located to the southeast of the huge walled plain Mendeleev, about midway between the craters Schliemann to the northeast and Marconi to the southwest. It is about the same size as Albategnius on the near side. The rim of this crater is roughly circular; however, the edge is uneven.
Observations of variations in the brightness of Io as it rotated, made by Joel Stebbins in the 1920s, showed that Io's day was the same length as its orbital period around Jupiter, thus proving that one side always faced Jupiter just as the Moon's near-side always faces the Earth. Stebbins also noted Io's dramatic orange coloration, which was unique among the Galilean satellites. Audouin Dollfus used observations of Io in the early 1960s at the Pic du Midi Observatory to create crude maps of the satellite that showed a patchwork of bright and dark spots across the Ionian surface, as well as a bright equatorial belt and dark polar regions. Telescopic observations in the mid-20th century began to hint at Io's unusual nature.
In the fall of 1879 volunteers for the expedition assembled their wagons, supplies, and livestock at a spring at the head of Fortymile Gulch, just south of the deep canyons of the Escalante River Basin, and just north of the cliffs of the Kaiparowits Plateau. A smaller group went ahead to find and prepare a crossing for Glen Canyon and the Colorado River. At Cottonwood Canyon they saw a tempting route up from the far side of the river and, on the near side, a narrow crevice that might allow a descent into the canyon. Naming it Hole-in- the-Rock, they proceeded to spend several months widening it for the passage of wagons, and building anchor points and tracks to assist with the descent.
Construction will occur from 2018 to 2020. Boarding islands are planned to be built at 30th Avenue; contrary to the original plan, the stops will remain on the near side of the cross street. A short high-level handicapped-accessible platform will be built on the inbound platform; its outbound counterpart will be at the otherwise closed 28th Avenue stop. Early implementation of some project elements, including painted clear zones where the outbound boarding island will be located, was done in early 2017. In response to merchants complaining about the loss of parking spaces to allow for boarding islands, the Board agreed to an experimental pilot program on the inbound side at five stops: 26th, 30th, 32nd, 35th, and 40th Avenues.
Moon - Evidence of young lunar volcanism (12 October 2014). The reason that the mare basalts are predominantly located on the near-side hemisphere of the Moon is still being debated by the scientific community. Based on data obtained from the Lunar Prospector mission, it appears that a large proportion of the Moon's inventory of heat producing elements (in the form of KREEP) is located within the regions of Oceanus Procellarum and the Imbrium basin, a unique geochemical province now referred to as the Procellarum KREEP Terrane. While the enhancement in heat production within the Procellarum KREEP Terrane is most certainly related to the longevity and intensity of volcanism found there, the mechanism by which KREEP became concentrated within this region is not agreed upon.
Flood in the nature sanctuary Altneckar The nature reserve Altneckar with its riparian forest and the adjacent grassland valley is an idyllic local recreational area and ecological oasis between the townships of Freiberg, Pleidelsheim, and Ingersheim. On the near side of the A 81 motorway the high railway embankment of the former railway line from Backnang to Bietigheim is protected and cared for by the town and the local committee of the BUND ("Union for the environment and nature conservation Germany") as a dry biotope. On the far side of A 81 the railway line cut a deep rut into the landscape. By the joint efforts of the town and the BUND there too a protective area was created, in the occurrence a dark moist wood biotope.
A study published in 2011 suggested that a subsequent collision between the Moon and one of these smaller bodies caused the notable differences in physical characteristics between the two hemispheres of the Moon. This collision, simulations have supported, would have been at a low enough velocity so as not to form a crater; instead, the material from the smaller body would have spread out across the Moon (in what would become its far side), adding a thick layer of highlands crust. The resulting mass irregularities would subsequently produce a gravity gradient that resulted in tidal locking of the Moon so that today, only the near side remains visible from Earth. However, mapping by the GRAIL mission has ruled out this scenario.
The second half opened with a sequence of three goals by both teams within five minutes, beginning with a short pass by Andy Williams to DaMarcus Beasley that was shot into the near side of the goal, cutting San Jose's lead to 2–1. Shortly after kickoff, a long overhead pass by Brian Mullan found Earthquakes midfielder Richard Mulrooney, who scored and restored the Earthquakes' two-goal lead. The Fire continued to press for a second goal and earned a throw-in near San Jose's goal that led to a cross into the box by Evan Whitfield. The cross was deflected into the goal by Earthquakes defender Chris Roner, who had been substituted three minutes earlier, narrowing the team's lead to 3–2 in the 54th minute.
In some places on Earth, there is only one high tide per day, whereas others such as Southampton have four, though this is somewhat rare. The notional tidal bulges are carried ahead of the Earth–Moon orientation by the continents as a result of Earth's rotation. The eccentric mass of each bulge exerts a small amount of gravitational attraction on the Moon, with the bulge on the side of Earth closest to the Moon pulling in a direction slightly forward along the Moon's orbit (because Earth's rotation has carried the bulge forward). The bulge on the side furthest from the Moon has the opposite effect, but because the gravitational attraction varies inversely with the square of distance, the effect is stronger for the near-side bulge.
Useful observation of the parts of the far side of the Moon occasionally visible from Earth is difficult because of the low viewing angle from Earth (they cannot be observed "full on"). The phrase "dark side of the Moon" does not refer to "dark" as in the absence of light, but rather "dark" as in unknown: until humans were able to send spacecraft around the Moon, this area had never been seen. While many misconstrue this to think that the "dark side" receives little to no sunlight, in reality, both the near and far sides receive (on average) almost equal amounts of light directly from the Sun. However, the near side also receives sunlight reflected from the Earth, known as earthshine.
Offensive tactics include improving a team's position on the ice by advancing the puck out of one's zone towards the opponent's zone, progressively by gaining lines, first your own blue line, then the red line and finally the opponent's blue line. NHL rules instated for the 2006 season redefined the offside rule to make the two-line pass legal; a player may pass the puck from behind his own blue line, past both that blue line and the centre red line, to a player on the near side of the opponents' blue line. Offensive tactics are designed ultimately to score a goal by taking a shot. When a player purposely directs the puck towards the opponent's goal, he or she is said to "shoot" the puck.
Luna 3, or E-2A No.1 () was a Soviet spacecraft launched in 1959 as part of the Luna programme. It was the first-ever mission to photograph the far side of the Moon and the third Soviet space probe to be sent to the neighborhood of the Moon. Though it returned rather poor pictures by later standards, the historic, never-before-seen views of the far side of the Moon caused excitement and interest when they were published around the world, and a tentative Atlas of the Far Side of the Moon was created after image processing improved the pictures. These views showed mountainous terrain, very different from the near side, and only two dark, low-lying regions which were named Mare Moscoviense (Sea of Moscow) and Mare Desiderii (Sea of Desire).
The phases of Venus, observed by Galileo in 1610 From September 1610, Galileo observed that Venus exhibits a full set of phases similar to that of the Moon. The heliocentric model of the Solar System developed by Nicolaus Copernicus predicted that all phases would be visible since the orbit of Venus around the Sun would cause its illuminated hemisphere to face the Earth when it was on the opposite side of the Sun and to face away from the Earth when it was on the Earth-side of the Sun. In Ptolemy's geocentric model, it was impossible for any of the planets' orbits to intersect the spherical shell carrying the Sun. Traditionally, the orbit of Venus was placed entirely on the near side of the Sun, where it could exhibit only crescent and new phases.
Partial view of excavated remains of Roman Fort Banna (at Birdoswald, Cumbria, England). Cohors I Ælia Dacorum was stationed here for at least 150 years until AD 276, and probably for about a century thereafter View of the remains of Hadrian's Wall (right, stretching into the distance), as seen from Fort Banna. Originally, the wall was c. 5 m (16 ft) high, but stone removal over the centuries has reduced its remains, at this point, to barely 2 m The regiment was transferred from Dacia to Britain not later than 125, when it was stationed briefly at Fort Fanum Cocidi (Bewcastle, Cumbria) and appears to have participated in the excavation of the so-called Vallum, a huge ditch running along the near side of Hadrian's Wall (constructed 122-8).
Before the team's next match at NYRB, Andrea Mancini was released to join the New York Cosmos, freeing up an international roster slot, and allowing the team to activate Kamara, who had sat out over six weeks with a hamstring injury. Without Acosta, United seemed hopelessly overmatched by the potent NYRB in a match scheduled to honor the 15th anniversary of the September 11 attacks. Indeed, the Red Bulls went ahead in the first half following a Nyarko defensive turnover that led to a historic goal by Bradley Wright-Phillips, giving BWP the most goals over a 3-year stretch by any player in league history. In the second half, Wright-Phillips caught Hamid leaning towards the far post and slammed it past him to the near side, giving NY a 2-0 lead.
General Yamashita (center, on the near side of the table) at the surrender ceremony at Camp John Hay on 3 September 1945. A major offensive to capture Baguio did not occur until April 1945, when the USAFIP-NL's 1st Battalion of the 66th Infantry, attached with the United States Army's 37th Infantry Division, the USAFIP-NL's 2nd Battalion of 66th Infantry, attached with the US 33rd Infantry Division, and the USAFIP-NL's 3rd Battalion of the 66th Infantry, converged on Baguio. By 27 April 1945, the city was liberated and the joint force moved on to liberate the Trinidad valley. Baguio is the site of the formal surrender of General Yamashita and Vice Admiral Okochi at Camp John Hay's American Residence in the presence of lieutenant generals Arthur Percival and Jonathan Wainwright.
After the success of the Battle of Morval and the Battle of Thiepval Ridge the Fourth Army was instructed on 29 September, to plan the capture of the area around Le Transloy, Beaulencourt and a ridge beyond the valley containing Thilloy and Warlencourt. The attack was to be ready by 12 October and be made in conjunction with attacks by the Reserve Army and the Third Army further north. Before the big offensive, the Fourth Army was to continue its attack to the north-east, to capture a spur short of Le Transloy and Beaulencourt and to the north to reach the near side of the Thilloy–Warlencourt valley. The Fourth Army had already ordered an advance on the left flank on 1 October, to capture Eaucourt and the Flers Line up to Le Sars.
Colonel Coughlin kept the gap under mortar and artillery fire for the rest of the night and ordered the Netherlands Battalion to send a company north from Hill 975 at first light to close it. General Ruffner directed the French Battalion to send a company up the valley from Putchaetful to clean out any PVA who sifted through the mortar and artillery barrages. Moving from Hill 975 toward Hill 1051 on the near side of the saddle, the Dutch company lacked the numbers to push through PVA who by daylight closed in around a platoon of Company A on the 1051 crest. The remainder of the Netherlands Battalion, under Colonel Coughlin's order, joined its forward company about 09:30, but, finding that Hill 1051 had fallen to the PVA, the Dutch commander, Lt. Col.
Geologic map of the near side of the Moon (high resolution, click to zoom) The lunar geological timescale (or selenological timescale) divides the history of Earth's Moon into five generally recognized periods: the Copernican, Eratosthenian, Imbrian (Late and Early epochs), Nectarian, and Pre-Nectarian. The boundaries of this time scale are related to large impact events that have modified the lunar surface, changes in crater formation through time, and the size-frequency distribution of craters superposed on geological units. The absolute ages for these periods have been constrained by radiometric dating of samples obtained from the lunar surface. However, there is still much debate concerning the ages of certain key events, because correlating lunar regolith samples with geological units on the Moon is difficult, and most lunar radiometric ages have been highly affected by an intense history of bombardment.
After capturing the legs with his arms and legs he begins rolling over to land on the mat. The spladle is a wrestling technique commonly used as a counter and pinning move to single leg take downs. When opponents shoot in and grab the leg the wrestler will drop their weight on the opponents head to prevent advancement of the take down, from there they may reach across the body with their arms to grab hold of the opponents far side leg, once completed they wrap the near side leg with the leg targeted for the take down and roll forward onto the mat. When on the floor it is important to control both legs of the opponent as the wrestler wants to bring the knees of his opponent as close to inline with the opponents head as possible.
The Last Supper (1445–1450) is a fresco by the Italian Renaissance artist Andrea del Castagno, located in the refectory of the convent of Sant'Apollonia, now the Museo di Cenacolo di Sant'Apollonia, and accessed through a door on Via Ventisette Aprile at the corner with Santa Reparata, in Florence, region of Tuscany. The painting depicts Jesus and the Apostles during the Last Supper, with Judas, unlike all the other apostles, sitting separately on the near side of the table, as is common in depictions of the Last Supper in Christian art. Sant'Apollonia was a Benedictine convent of cloistered nuns, and Castagno's fresco was not publicly known until the convent was suppressed in 1866: Vasari, for example, seems not to have known of the painting.John Spencer, Andrea Del Castagno and His Patrons, Durham: Duke University Press, 1991, pp. 102-111.
To insert the bit into the horse's mouth, the groom should stand on the near side of the horse, place the reins over the animal's head, and raise the headstall in his right hand while directing the bit to the horse's mouth with his left. If the horse refuses the bit, the groom should hold the bit against the horse's teeth with his fingers, and insert his left thumb in the horse's jaws. If the horse still refuses, the groom should press the animal's lips against his canine tooth, which should make the horse open his mouth. Here Xenophon suggests that the horse be bitted not only before he is to be worked, but also before he is fed and led home from a ride, so that he does not necessarily associate the bit with discomfort and labor.
The probe was previously planned for launch by a Long March 5 rocket at the Wenchang Satellite Launch Center on Hainan Island, but a failure of this vehicle in 2017 created uncertainty about its ability to carry Chang'e 5. The spacecraft is still planned to be launched with a Long March 5 rocket, and the planned landing zone is Mons Rümker in Oceanus Procellarum, located in the northwest region of the near side of the Moon. The location is a large, elevated volcanic mound 70 km in diameter that features a strong spectroscopic signature of basaltic lunar mare material. The mission is reported to consist of four modules or elements: the lander would collect about of samples from below the surface and place them in an attached ascent vehicle that will be launched into lunar orbit.
The Lagrange point of the Earth–Moon system is located about above the far side, which has also been proposed as a location for a future radio telescope which would perform a Lissajous orbit about the Lagrangian point. One of the NASA missions to the Moon under study would send a sample-return lander to the South Pole–Aitken basin, the location of a major impact event that created a formation nearly across. The force of this impact has created a deep penetration into the lunar surface, and a sample returned from this site could be analyzed for information concerning the interior of the Moon. Because the near side is partly shielded from the solar wind by the Earth, the far side maria are expected to have the highest concentration of helium-3 on the surface of the Moon.
Luna 3 phototelegraph system at Tsiolkovsky State Museum of the History of Cosmonautics The first view returned by Luna 3 showed the far side of the Moon was very different from the near side, most noticeably in its lack of lunar maria (the dark areas) The purpose of this experiment was to obtain photographs of the lunar surface as the spacecraft flew by the Moon. The imaging system was designated Yenisey-2 and consisted of a dual-lens camera AFA-E1, an automatic film processing unit, and a scanner. The lenses on the camera were a 200 mm focal length, f/5.6 aperture objective and a 500 mm, f/9.5 objective. The camera carried 40 frames of temperature- and radiation- resistant 35 mm isochrome film. The 200 mm objective could image the full disk of the Moon and the 500 mm could take an image of a region on the surface.
He was 37 years old, and an Acting Lieutenant-Colonel in the Norfolk Regiment, British Army, Commanding Officer 1st Battalion, Royal Inniskilling Fusiliers during the First World War when the following deed took place for which he was awarded the VC. On 20 November 1917 during the Battle of Cambrai at Marcoing, France, when a party of men were held upon the near side of a canal by heavy rifle fire, Lieutenant Colonel Sherwood Kelly at once ordered covering fire, personally led his leading company across the canal and then reconnoitered, under heavy fire, the high ground held by the enemy. He took a Lewis gun team, forced his way through obstacles and covered the advance of his battalion, enabling them to capture the position. Later he led a charge against some pits from which heavy fire was coming, capturing five machine-guns and 46 prisoners.
If the line there was overrun, the enemy would be able to fire into the rear of the troops deployed along the railway in both directions. Despite this, the Australian commanders considered it important to hold the railway line; if it was not garrisoned, the enemy could assemble in the dead ground behind the embankment. A further difficulty arose from the fact that if an attack occurred during daylight, it would be almost impossible to move troops down the exposed slopes to reinforce the railway line without crippling losses, and troops withdrawing from the railway line would be similarly exposed. To afford them some protection along the railway line, the forward posts dug one-man niches in the near side of the embankment, but the only way for them to fire was to climb up and lie on top of the embankment, thus exposing themselves to enemy fire.
Nearside car 6618 at the Seashore Trolley Museum in Kennebunkport, ME The Nearside (or Near-side) Car was a streetcar (trolley car or tram) designed by in-house engineers of the Thomas E. Mitten management team, which ran the Philadelphia Rapid Transit Company (PRT). Nearside refers to the fact the car would pick up and discharge passengers on the “nearside” of an intersection rather than the “farside” as the previous generation of “conventional” cars did (this method of operation caused frequent gridlock, as the stopped cars blocked cross traffic). The 1,500 cars that the PRT ordered from the J. G. Brill Company in South Philadelphia was the largest single order of streetcars in North American history.Brill, Debra, History of J G Brill Company,Indiana University Press, Bloomington, IN, 2002 The cars were initially designed as “muzzle loaders” with only double front doors for passenger entry and exit.
The Mabuiag, or Mabuygiwgal, are an Indigenous Australian group of Torres Strait Islander people united by a common language, strong ties of kinship and survived as skilled hunter–fisher–gatherers in family groups or clans living on a number of Torres Strait Islands including Mabuiag Island, in the Torres Strait in Queensland, Australia. They are ethnically Melanesian. They in common with all Torres Strait Islanders had a mixed reputation for hostility as well as eagerness to develop trading links with outsiders before they became Christian in the early 1870s. The language of the island is Mabuiag, a dialect of Kala Lagaw Ya. The society consists of two moieties ("koey buway"), the Mabuygiw people of Wagedagam ('Rear-Side') on the northwest (kukidagam) side of Mabuiag (their totem wind and direction), and the Mabuygiw people of the Panay ('Near-Side') on the south-east side (sagerdagam), their main totem wind and direction.
In some classifications, they are a parallel region to the Pacific Ranges rather than its subdivisions, and in others they are part of the Chilcotin Plateau. That is to say, part of the Interior Plateau, along with the Marble Range and Clear Range on the other side of the Fraser River from it. In such a classification system, the boundary of the Chilcotin Ranges would stop at the Yalakom River, the North Fork of the Bridge River, which is the western boundary of the Camelsfoot. On the other hand, those ranges, classified as part of the Interior Plateau, are really part of the same geologic system as the Coast Mountains across the Fraser or the Cascade Range south of the Thompson on the near side of the Fraser, which has been riven by the gorges of the Thompson and Fraser Canyons to separate the Pacific Cordillera into different ranges.
The Topographic Globe of the Moon Geological features of the Moon (near side / north pole at left, far side / south pole at right) alt=Topography of the Moon measured from the Lunar Orbiter Laser Altimeter on the mission Topography of the Moon STL 3D model of the Moon with 10× elevation exaggeration rendered with data from the Lunar Orbiter Laser Altimeter of the Lunar Reconnaissance Orbiter The topography of the Moon has been measured with laser altimetry and stereo image analysis. Its most visible topographic feature is the giant far-side South Pole–Aitken basin, some in diameter, the largest crater on the Moon and the second-largest confirmed impact crater in the Solar System. At deep, its floor is the lowest point on the surface of the Moon. The highest elevations of the surface are located directly to the northeast, and it has been suggested might have been thickened by the oblique formation impact of the South Pole–Aitken basin.
This variety of features is easy to spot with a variety of window placement and sizes, while Observation Car windows tend to be more uniform in size and placement. Among North American railroads, their observation cars often featured any of a variety of upcharge revenue seating, reserved sitting/drawing rooms or sleeper roomettes in the forward section, in the form of reclining coach seats, plush parlor car chairs near side tables or bedrooms and the occasional crew dormitory, such configurations varying greatly between railroads. A lighted drumhead adornment, usually indicating the name of the train or the name/logo of the railroad would invariably (except on the Milwaukee Road, see below) be hung from the tail end of the observation car. Some early trains offered two observation cars: a traditional enclosed type for its compartment or "first class" passengers and an open type resembling a flat car for its tourist class riders.
Its surface was orange in color and marked by dark spots, which were initially interpreted as the sites of impact craters. Among the most intriguing features was a heart-shaped, dark ring across that would later turn out to be the plume deposit of the volcano Pele. The data from the Ultraviolet Spectrometer (UVS) revealed a torus of plasma composed of sulfur ions at the orbit of Io, but tilted to match the equator of Jupiter's magnetic field. The Low-Energy Charged Particle (LECP) detector encountered streams of sodium, sulfur, and oxygen ions prior to entering Jupiter's magnetosphere, material that the LECP science team suspected originated from Io. In the hours prior to Voyager 1's encounter with Io, the spacecraft acquired images for a global map with a resolution of at least per pixel over the satellite's leading hemisphere (the side that faces the moon's direction of motion around Jupiter) down to less than per pixel over portions of the sub-Jovian hemisphere (the "near" side of Io).
Horse led from the side, excess lead rope folded and held, not wrapped around the hand Wrapping the lead rope around the hand can have disastrous consequences By tradition, the handler leads a horse from the horse's left ("near") side, though situations may arise when a horse needs to be led from the right ("off") side. In some areas, particularly in the American west, the handler may be in front of the horse while leading, though this technique does place the handler at risk due to not being able to see what the horse is doing. When leading a horse, the handler usually holds a single thickness of the lead with the right hand, while carrying the gathered slack of the lead in the left. The excess line should be laid in back-and-forth loops that fall on either side of the hand; holding the excess in circular loops, wrapping, or coiling the lead around the hand is dangerous, the handler can be dragged, injured or even killed if the horse pulls away, tightening the loops of the lead around the hand.
Below is a basic method of tying. The knot can also be made by using the rod itself to form the loop, but the tying method does not affect the performance of the resulting hitch. Begin with an overhand loop, that is, a loop in which the working part passes over the standing part: 350px Fold the loop over the working part, towards the standing part such that the standing part is visible through the center of the loop: 350px In stiffer material the first two steps can be accomplished in a single motion by twisting the working part with the fingers until a loop forms and flops over the standing part. Use the rod to snag a bight of the standing part through the loop, that is, pass the rod over the near side of the loop, under the standing part and then over the far side of the loop: 350px Before tensioning, excess slack can be removed by pulling simultaneously on both the working and standing parts: 350px In actual use the hitch should be loaded only from the standing side.
After a first series, a green synchro light was fitted at the lower right edge of the platter to indicate the reaching of the nominal rotational speed. The external illumination ‘pod’ was available as an option, and was mounted on the left near side of the deck. EMT 938 Turntable The ‘948’ cost around DM 12000 and was therefore still too expensive for many professional users. (For many customers in faraway countries, it was also too complicated, so EMT continued the production of the ‘930’ until 1982.) An even smaller and cheaper unit was designed and introduced in March, 1982: the ‘938’ ‘Broadcast Disk Reproducer’ (Rundfunk-Plattenspieler) featured a simplified direct-drive and electronics, it was slimmer and cheaper than its two brothers and some of its parts, like the plinth and lid, were taken from commercial ‘hi-fi’ products. The 938 had been designed in co-operation with Thorens, and a modified version of the 938 was marketed by this firm as the ‘TD 524’, a discothèque-oriented deck that could be equipped with a Thorens ‘TP 16L’ or even the EMT ‘929’ tonearm.

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