How Do Binary Stars Orbit and Affect Each Other's Mass and Distance?

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SUMMARY

In a binary star system where two stars orbit each other with a period of 30 days and a velocity of 30 km/s, both stars have equal mass due to their identical distance from the center of mass. The gravitational relationship can be expressed using the equation 1/2mV^2 = (-gMm)/r, where 'm' represents the mass of each star and 'r' is the radius from the center of mass. The discussion highlights the application of Kepler's laws and the importance of understanding the center of mass in binary systems.

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  • Basic principles of orbital mechanics
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EbolaPox
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Two stars in a binary system orbit each other with a period of 30 days. Each moves with velocity 30 km/s. A) What is the mass of each, and B) their separation.

Ok, First thing I noticed was w*r=v this would mean though that the stars are the same distance from the center of mass. I used this radius and calculated the mass of the stars using 1/2mV^2=(-gMm)/r.

If the radius from the center of mass is equal for both stars that means that they would both have to be the same mass. I tried to use the center of mass equation and something relating to gravity to isolate just one variable and solve but couldn't come up with anything. Then I drew another picture for myself and realized that since they are both traveling at the same tangental velocity at the same period they are traveling the same distance. Does this make sense to anyone else? Or am I way off the mark. I wanted to try and use kepler's laws but had too many variables. Any ideas suggestions?
 
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I agree. They would be circling the same path.
 

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