This is a series of analysis of Angular velocity as relates to an asteroid's orbit. See the explanation below.
<h3>What is an asteroid?</h3>
Asteroids are stony bodies that circle the Sun.
Although asteroids circle the Sun in the same way as planets do, they are far smaller.
Hence, from the information given:
A) The square of the period is proportional to the cube of the semimajor axis, according to Kepler's third law. As a result, the period of Y equals (E) the period of Z.
B) Angular momentum is preserved here, hence it is equivalent (E).
C) As eccentricity increases, so does the angular momentum. In this case, Y and Z have the same period, and both satellites cover the same proportion of the territory in the same length of time.
This indicates that a satellite on Z must cover a lesser area in a given period of time than a satellite on Y. The area swept is approximately 1/2 the radius times the tangential displacement.
Because both satellites have the same "radius" at point y, the satellite on Z must have a lower tangential velocity than the one on Y. As a result, Y has more angular momentum than (G) Z.
D) Using Kepler's third law, X's period is bigger than (G) Z's.
E) In a circular orbit, the angular velocity is constant. As a result, the angular velocity of Y at y equals (E) that at s.
F) Z's angular velocity at c is smaller than (L) at i.
G) Y's angular velocity at y is larger than (G) Z's at y.
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