Find mass of black hole in center of galaxy given eccentricity+

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SUMMARY

The discussion centers on calculating the mass of a black hole at the center of the Milky Way galaxy using the observed star "S2," which has a 15.2-year orbital period, an eccentricity of 0.87, and a semimajor axis of 4.62 mpc. The mass is derived using the formula Mass = (4π²r³) / (GT²), where r is the average of the semi-major and semi-minor axes. The initial calculation of r was incorrect, leading to an erroneous mass of 3.11 x 10^36 kilograms, which was later corrected to 1.426 x 10^11 km, yielding the correct mass that confirms the presence of a black hole based on its density relative to its size.

PREREQUISITES
  • Understanding of orbital mechanics and Kepler's laws
  • Familiarity with the concepts of eccentricity and semi-major axis
  • Knowledge of gravitational physics, specifically Newton's law of gravitation
  • Ability to perform calculations involving units of distance such as parsecs and milli-parsecs
NEXT STEPS
  • Study the implications of black hole density and its relationship to mass
  • Learn about the methods used to observe and measure stellar orbits around supermassive black holes
  • Explore the significance of eccentricity in orbital dynamics
  • Investigate the role of gravitational interactions in galaxy formation and evolution
USEFUL FOR

Astronomers, astrophysicists, and students studying celestial mechanics or black hole physics will benefit from this discussion, particularly those interested in the dynamics of stars around supermassive black holes.

oddjobmj
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Homework Statement


Astronomers believe that there is a massive black hole at the center of the Milky Way galaxy. What evidence is there for that?
A group of astronomers have observed a star "S2" in a 15.2-year orbit around the center of the galaxy. They measured the period of revolution T = 15.2 years, the eccentricity of the elliptical orbit ε = 0.87, and the semimajor axis of the orbit a = 4.62 mpc. [The unit: mpc = milli-parsec = 0.001 parsec.]

(A) Calculate the mass of the compact object about which S2 is revolving.


Homework Equations



sm=semi-minor axis
sM=semi-major axis

Eccentricity=\sqrt{1-(sm/sM)^2}

Mass=\frac{4π^2r^3}{GT^2}

The Attempt at a Solution



If I plug in my values to the eccentricity equation and solve for the semi-minor axis I get 7.031*1010 km. With that I can find r which is the average of the semi-major and semi-minor axis:

r=1.06455*1011 km

Plugging in my knows to the mass equation I get 3.11*10^36 kilograms which is incorrect. What am I doing wrong?

Thank you!
 
Physics news on Phys.org
Apparently the way I figured out r was incorrect. It should be 1.426 *10^11 km. My answer is now correct!
 
Why does the correct mass imply its a black hole? Density from known size?
 

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