UNIVERSE LL W/SAPLINGPLUS MULTI SEMESTER
UNIVERSE LL W/SAPLINGPLUS MULTI SEMESTER
11th Edition
ISBN: 9781319278670
Author: Freedman
Publisher: MAC HIGHER
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Chapter 8, Problem 36Q
To determine

The radial velocity method that is used to detect planets orbiting other stars. Also, provide the reason for difficulty in using this method to detect planets like Earth.

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Nearly all planets that astronomers have found orbiting other stars have been giant planets with masses more like Jupiter than Earth, and with orbits located very close to their parent stars. Does this prove that our Solar System is unique? Explain your answer.
A certain binary system consists of two stars that have equal masses and revolve in circular orbits around a fixed point half-way between them.   If the orbital velocity of each star is v=186 km/s and the orbital period of each is 11.3 days, calculate the mass M of each star. Give your answer in units of the solar mass,  1.99×1030 kg (e.g. if each planet's mass is 3.98×1030 kg, you would answer "2.00").
The figure below shows the radial velocity of a star plotted as a function of time over the course of 20 days. Where is the planet in its orbit around the star when the star's radial velocity is 18 km/s? How do I determine this?
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