Gravity and the Rotation of Galaxies

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SUMMARY

This discussion focuses on the relationship between gravity and the rotation of galaxies, specifically addressing the lab questions regarding observed speeds and mass estimation methods. The equation v = √(Gmg/r) is referenced to explain observed speeds, with the conclusion that variations in G can lead to different results. Astronomers typically estimate galaxy mass using virial theory and determine radius through observational data, acknowledging that these methods yield approximate values.

PREREQUISITES
  • Understanding of gravitational equations, specifically v = √(Gmg/r)
  • Familiarity with virial theory for mass estimation
  • Knowledge of observational techniques in astronomy
  • Basic comprehension of the gravitational constant (G)
NEXT STEPS
  • Research the application of virial theorem in astrophysics
  • Explore observational methods for measuring galaxy radius
  • Study the implications of varying the gravitational constant (G) in cosmology
  • Learn about the dynamics of galaxy rotation curves and dark matter
USEFUL FOR

Astronomy students, astrophysicists, and anyone interested in understanding galaxy dynamics and the effects of gravity on rotational speeds.

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hey i need help! We are doing a lab on the above title and I have no idea how to do it.
So there are few questions i wanted to know to ace this lab. lol i will really appreciate it if someone can help me.

- Describe the differences between the two sets of data. Is the observed speeds explained by the equation
v = √Gmg/ r ? Justify your answer

-Briefly describe some of the methods astronomers use to estimate the mass of a galaxy, its radius and the value of G.


Please, it will be really helpful if someone can help me!
 
Astronomy news on Phys.org
Galaxy mass, usually by virial theory. Radius by observation. Both methods are approximate. G is assumed. Wiggle G and any result is possible.
 

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