Solve Mass of Star Problem: Astronomy Class Final Year

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SUMMARY

The discussion centers on solving the mass of a star problem for a final year astronomy class. The correct expression for the density of a star is given as ρ(r) = ρ_{c}(1 - (r/R)^{3}), indicating that density varies throughout the star's volume. To derive the mass M(r) and the total mass, integration techniques are essential. The initial assumption regarding the volume of a sphere and density was incorrect due to the non-constant nature of stellar density.

PREREQUISITES
  • Understanding of spherical volume calculations
  • Familiarity with density functions in astrophysics
  • Basic integration techniques in calculus
  • Knowledge of stellar structure and composition
NEXT STEPS
  • Study integration methods for variable density functions
  • Research the concept of stellar density profiles
  • Learn about the derivation of mass in astrophysical contexts
  • Explore applications of the equation of state in stellar physics
USEFUL FOR

Astronomy students, astrophysicists, and educators seeking to understand stellar mass calculations and density variations in stars.

jimmyd
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hi, this is my first post here as i have driven insane by a math problem for my final year astronomy class, I've been at it for 3 hours and i can't make sense of it

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is the question even correct as i have made the assumption that the volume of a sphere times the density would give me 4 were there is a 2 and the density p instead of the density constant pc?
 
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The density of the star is not constant throughout its volume. The expression for the density in section (1a) should be written

ρ(r) = ρ[itex]_{c}[/itex](1 - (r/R)[itex]^{3}[/itex])

for clarity. In order to derive M(r) and the total mass, you must do some integrations.
 

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