{[ promptMessage ]}

Bookmark it

{[ promptMessage ]}

The Masses of Star1 - The Masses of Stars Note of caution...

Info iconThis preview shows page 1. Sign up to view the full content.

View Full Document Right Arrow Icon
The Masses of Stars Note of caution about comparisons: When comparing two separate binary systemS of the same separation distance, the two stars in the binary system that has larger combined mass will move faster than the two stars in the binary system with less combined mass. The larger combined mass binary has greater gravity force acting between the two stars. When comparing the two stars within a particular binary system, the larger mass star will move slower than the less massive star. The gravity force acting on the two stars within the binary is the same for both of the stars. The distance travelled by an object = velocity × the time it takes. The distance travelled by the star is just the circumference of the orbit = 2 π × the radius of a circular orbit and something similar for an elliptical orbit. Therefore, each star's C.M.-distance r = the star's velocity × the star's orbital period / (2 π ). This allows you to use the easily measured velocity in Kepler's third law and in the center of mass relations.
Background image of page 1
This is the end of the preview. Sign up to access the rest of the document.

{[ snackBarMessage ]}