Help with Doppler shift galaxy question

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SUMMARY

The discussion centers on solving a physics problem involving the Doppler shift of a star's spectrum, which indicates it is orbiting an 'invisible companion'. Key parameters include a sinusoidal velocity amplitude of 90 m/s and a period of 10^6 seconds. The participant seeks to determine the mass of the companion star and the distance between the two stars during an eclipse. The Virial Theorem and orbital mechanics are essential tools for deriving these values from the provided data.

PREREQUISITES
  • Doppler shift analysis in astrophysics
  • Understanding of the Virial Theorem
  • Orbital mechanics and Kepler's laws
  • Basic stellar dynamics and mass estimation techniques
NEXT STEPS
  • Study the application of the Virial Theorem in binary star systems
  • Learn about the Two-body Problem in celestial mechanics
  • Explore methods for calculating the mass of celestial bodies using orbital parameters
  • Investigate the relationship between Doppler shift and orbital velocity
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Astronomy students, astrophysicists, and educators seeking to understand binary star systems and the application of Doppler shift in determining stellar masses.

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Homework Statement


Hi, I'd really appreciate being pointed in the right direction with this past exam question, as I just have no idea how to approach it and can't find similar examples in my notes anywhere.
A nearby star has a spectrum similar to the sun, suggesting it has the same mass. The Doppler shift of lines in the stellar spectrum vary sinusoidally with a period of 10^6s and velocity amplitude of 90m/s

The question then asks for things like the mass of the 'invisible companion' to the star, and then lead onto finding the distance from one star to the other as they eclipse, etc.

What I'm really asking, is what information can I get using the period, velocity amplitude, and mass?

Any help appreciated!

Homework Equations


Can the Virial Theorem be used?
(1/2)I''=2U+Ω where I= Σmr^2, U is kinetic energy and Ω is potential energy.
v=(2pia)/P I could find the velocity of the galaxy if I knew the semi major axis, then maybe combine this with the doppler shift information given in the question?

The Attempt at a Solution


Some ideas above..
 
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What I'm really asking, is what information can I get using the period, velocity amplitude, and mass?
The doppler shift tells you something about the speed of the star - the fact that the doppler shift is periodic tells you the star is orbiting something.
You may need to make some guesses about the orbit - but if you know the orbit-speed and you know the orbit period, then you should be able to figure out the likely mass of the primary. How would you normally do this?

What you don't want to do is try to guess the "right" equation to use.
Note: this is not a "doppler shift galaxy" question.
 

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