21. Plaskett's binary system consists of two stars that reolve in a circular orbit about a center of mass midway between them. This statement implies that the masses of the two stars are equal (Fig. P13.21). Assume the orbital speed eof each star is of each is 14.4 days, Find the mass M of each star. (For comparison, the mass of our Sun is 1.99 x 1030 kg.) = 220 km/s and the orbital period M *CM Figure P13.21
21. Plaskett's binary system consists of two stars that reolve in a circular orbit about a center of mass midway between them. This statement implies that the masses of the two stars are equal (Fig. P13.21). Assume the orbital speed eof each star is of each is 14.4 days, Find the mass M of each star. (For comparison, the mass of our Sun is 1.99 x 1030 kg.) = 220 km/s and the orbital period M *CM Figure P13.21
College Physics
11th Edition
ISBN:9781305952300
Author:Raymond A. Serway, Chris Vuille
Publisher:Raymond A. Serway, Chris Vuille
Chapter1: Units, Trigonometry. And Vectors
Section: Chapter Questions
Problem 1CQ: Estimate the order of magnitude of the length, in meters, of each of the following; (a) a mouse, (b)...
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21

Transcribed Image Text:21. Plaskett's binary system consists of wo stars that revolve
in a circular orbit about a center of mass midway between
them. This statement implies that the masses of the two
stars are equal (Fig. P13.21). Assume the orbital speed
eof each star is
of each is 14.4 days, Find the mass M of each star. (For
comparison, the mass of our Sun is 1.99 x 100 kg.)
= 220 km/s and the orbital period
M
*CM
Figure P13.21
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