Binary star system distance between stars

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SUMMARY

The discussion centers on calculating the distance between two stars in a binary star system with a period of 90 days and each star having a mass of twice that of the Sun. The correct approach involves using the gravitational force equation, specifically F = GM^2/(2r)^2, where M is the mass of one star and r is the distance to the center of mass. The misunderstanding arises from the incorrect application of the distance in the gravitational force equation, where the distance between the stars is actually 2r, not r.

PREREQUISITES
  • Understanding of Newton's law of gravitation
  • Familiarity with centripetal force concepts
  • Knowledge of binary star systems and their dynamics
  • Basic algebra for solving equations
NEXT STEPS
  • Study the derivation of gravitational force equations in binary systems
  • Learn about the concept of center of mass in multi-body systems
  • Explore the implications of Kepler's laws on binary star systems
  • Investigate the effects of mass and distance on gravitational interactions
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Astronomy students, astrophysicists, and anyone interested in understanding the dynamics of binary star systems and gravitational interactions.

frostking
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Homework Statement


A binary star system has a period of 90 days. It consists of two equally massed stars each with a mass of twice that of the sun, that rotate like a dumbbell about the center of mass at the midpoint between them. How far apart are these stars?


Homework Equations


F = ma v = 2 pi r/T force of g = GMm/r^2 distance = 2r




The Attempt at a Solution


I set GMm/r^2 = m v^2/r then solve for r and d is 2 r. My problem is that my solution sheet uses force of g = GM^2/(2r)^2 and then force = to M v^2/r I know this has something to do with the fact that we have two stars and therefore, I guess M times M but I am confused... Could someone please explain why the equations used in the solution sheet are the correct ones and why in turn mine are incorrect? Thanks, Frostking
 
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frostking said:

The Attempt at a Solution


I set GMm/r^2 ...my solution sheet uses force of g = GM^2/(2r)^2

You used r^2 where the distance between them is 2r, they are orbiting about a common center of mass.
 
Both stars revolve around their common centre of mass which is halfway between them, at distance r, so the centripetal force is mv2/r, but the other star is 2r distance apart, so the gravitational interaction between the stars is Gm2/(2r)2.

ehild
 

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