What does momentum conservation reveal about period and mass of binary systems?

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SUMMARY

The discussion focuses on the principles of momentum conservation in binary star systems, specifically addressing why total momentum remains constant and the implications for the stars' positions and mass. The total momentum of the binary system, defined as p = m1 x v1 + m2 x v2, is conserved due to the absence of external forces. The stars must be diametrically opposite to maintain constant net momentum, and this configuration leads to a common period of rotation, with the inner star being the more massive of the two due to gravitational dynamics.

PREREQUISITES
  • Understanding of Newton's laws of motion
  • Familiarity with gravitational forces and their effects
  • Basic knowledge of binary star systems
  • Concept of momentum and its conservation
NEXT STEPS
  • Study the principles of Newtonian mechanics in binary systems
  • Explore gravitational interactions in astrophysics
  • Learn about the dynamics of rotating systems
  • Investigate the mass-luminosity relationship in stars
USEFUL FOR

Astronomy students, astrophysicists, and educators seeking to deepen their understanding of binary star dynamics and momentum conservation principles.

FelixISF
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Homework Statement


A binary star consists of two stars that are orbiting a common centre. The only force acting on the stars is the gravitational force of attraction in a direction along the line joining the stars.

a) Explain carefully why the total momentum of the binary is constant.

b) Explain why the two stars are always in a diametrically opposite position.

c) Hence explain why the two stars have a common period of rotation and why the inner star is the more massive of the two.


Homework Equations



No equations needed.



The Attempt at a Solution



a) The total momentum p = m1 x v1 + m2 x v2. Since there are no external forces acting on the binary system, momentum is by definition conserved.

--> Does that also imply that the momentum is constant? Because I think that the momentum could vary during one complete revolution and still be conserved right?

b) They must be in a diametrically opposite position in order for their velocity vectors to have opposite directions. If the were not diametrically opposite, the net momentum would not be constant.

c) I have no clue here..
 
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A quick hint'd suffice..
 

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