Calculating the Mass of a Binary Star System

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SUMMARY

The discussion focuses on calculating the mass of a binary star system, specifically using the masses m1=6*1.99*10^30 kg and an orbital period T=1.7 days. The participants utilize the gravitational force equation G*m1*m2/(r1+r2)^2 = m1(2π/T)^2*r1 to derive the mass of the second star, m2. The challenge lies in determining the radius r2, as both stars share the same orbital period. The conversation emphasizes the need for additional equations to solve for the three unknowns involved in the calculations.

PREREQUISITES
  • Understanding of gravitational force equations in astrophysics
  • Familiarity with binary star systems and their dynamics
  • Knowledge of orbital mechanics and Kepler's laws
  • Basic proficiency in algebra for solving equations
NEXT STEPS
  • Study the gravitational force equations in detail, focusing on G*m1*m2/(r1+r2)^2
  • Learn about Kepler's laws of planetary motion and their application to binary stars
  • Explore methods for calculating orbital radii in binary systems
  • Investigate the characteristics of different types of stars, particularly compact and dense stars
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Astronomy students, astrophysicists, and anyone interested in the dynamics of binary star systems and gravitational calculations.

coltsamuel96
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mass of a star...

given is a binary star system, with mass m1=6*1.99*10^30kg, radius =r1, v=270km/s, orbital period, T=1.7days... the other star of the binary system(compact and dense)with mass m2, and radius r2 orbits around a same common point... (r1>r2, G=6.67*10^-11Nm^2kg^-2) calculate, 1.)approximate mass of m2 2.)what type of star is m2?
attempt at the question, i used this equation, G*m1m2/(r1+r2)^2=m1(2pi/T)^2*r1 and furthermore i did, v=r(2pi/T), with this i get r1... but how do i get r2?so that i can get m2 from the above equation of G*m2/(r1+r2)^2=(2pi/T)^2*r1
 
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Did you know the period is the same for both stars?
I was convinced by looking at the animation in Wikipedia (binary stars).
And, of course, the force. Anyway, you can write that
F = 4π²m1*r1/T² = 4π²m2*r2/T².
That gives you 2 equations and 3 unknowns, I think. Maybe use the other formula for the force in the same way to get a 3rd equation?
 

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