21st Century Astronomy
21st Century Astronomy
6th Edition
ISBN: 9780393428063
Author: Kay
Publisher: NORTON
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Chapter 4, Problem 22QP
To determine

Find the observational quantities needed to make estimate an object’s mass.

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Why are all large celestial bodies (stars, planets, larger moons) very nearly spherical in shape?   a because of the centrifugal force from the body's rotation   b because of tidal forces   c because gravity tries to pull every part of the celestial body to the center   d because of the pressure from the heat in the body's core
Use Kepler's 3rd Law and the small angle approximation. a) An object is located in the solar system at a distance from the Sun equal to 41 AU's . What is the objects orbital period? b) An object seen in a telescope has an angular diameter equivalent to 41 (in units of arc seconds).  What is its linear diameter if the object is 250 million km from you?  Draw a labeled diagram of this situation.
Could you find the Mass of the Sun using the slope of the of T2 versus a3, using the values that are in units of years and AU? Explain
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