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"apocenter" Definitions
  1. the point of an orbit farthest from the center of attraction
"apocenter" Synonyms
"apocenter" Antonyms

5 Sentences With "apocenter"

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

The diagram illustrates the orbits of Neptune's irregular moons excluding Triton. The eccentricity is represented by the yellow segments extending from the pericenter to apocenter with the inclination represented on Y axis. The moons above the X axis are prograde, those beneath are retrograde. The X axis is labeled in Gm and the fraction of the Hill sphere's radius.
At apocenter, the satellite is more than 72 Gm from Neptune. This distance is great enough to exceed Mercury's aphelion, which is approximately 70 Gm from the Sun. Neso is also the moon with the longest orbital period, 26.67 years. It follows a retrograde, highly inclined, and highly eccentric orbit illustrated on the diagram in relation to other irregular satellites of Neptune.
A number of X-ray sources, likely X-ray binary stars, within the galaxy's central region appear as yellowish dots. The blue source at the center is at the position of the supermassive black hole. It has been proposed that the observed double nucleus could be explained if P1 is the projection of a disk of stars in an eccentric orbit around the central black hole. The eccentricity is such that stars linger at the orbital apocenter, creating a concentration of stars.
3 Piscis Austrini, also known as HD 201901, is a suspected astrometric binary star system that, despite its Flamsteed designation, is actually located in the constellation Microscopium. It is visible to the naked eye as a faint, orange-hued star with an apparent visual magnitude of 5.41. The system is moving closer to the Earth with a heliocentric radial velocity of −46 km/s. It is following a highly elliptical orbit around the Galactic Center, moving between a pericenter of out to an apocenter of , with an orbital eccentricity of 0.49.
From the above definitions, a new quantity, M, the mean anomaly can be defined :M = n(t - \tau), which gives an angular distance from the pericenter at arbitrary time t, with dimensions of radians or degrees. Because the rate of increase, n, is a constant average, the mean anomaly increases uniformly (linearly) from 0 to 2 radians or 0° to 360° during each orbit. It is equal to 0 when the body is at the pericenter, radians (180°) at the apocenter, and 2 radians (360°) after one complete revolution.Meeus (1991), p.

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