How Do I Calculate Galactic Mass Proportional to Radius?

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To calculate galactic mass as a function of radius, the equations M(r)=v^2r/G and M(r)=vrc^2/G are discussed, with the first being the correct formula for calculating mass based on velocity and radius. The velocity, v, can be determined from the flat rotation curve by using the total mass and radius of the galaxy. For tidal force calculations, the derived formula r=(d^3m/(2MR))^1/2 is presented, where m is the mass of the galaxy containing the star, R is its radius, M is the mass of the nearby galaxy, and d is the distance between the galactic centers. Verification of these calculations is sought to ensure accuracy. Understanding these relationships is crucial for analyzing galactic dynamics and tidal interactions.
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How do I calculate galactic mass as a function of r? I know it is supposed to be proportional to r. I've seen,
M(r)=v2r/G
And also I've seen
M(r)=vrc2/G
Which if any is right?
And what do I use for v?
Thanks so much for your help!
 
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The rotation curve is flat so I can find v by plugging in the radius and total mass of the galaxy. Doing that I get,
M(r)=Mr/R, where M is the total mass of the galaxy and R is the radius of the galaxy
I'm trying to do a tidal force calculation to see how far away from the center of a galaxy a star needs to be to be tidally disrupted by a nearby galaxy. I'm getting
r=(d3m/(2MR))1/2 where m is the total mass of the galaxy that the star lies in, R is the radius of that galaxy, M is the total mass of the nearby galaxy, and d is the distance between the two galactic centers. Can anyone verify this?
 
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