ValarDohaeris
- 3
- 0
The discussion revolves around the addition of gravitational potentials and orbital velocity, particularly in the context of mass distribution influenced by dark matter. Participants are exploring the integration of density functions to determine mass contributions in a gravitational context.
Some participants have provided insights into the integration process and the need to account for multiple mass terms. There is an ongoing exploration of the correct interpretation of the problem and the relationships between the variables involved.
Participants are navigating potential misunderstandings regarding the definitions of mass terms and the integration limits, indicating a need for clarity on the problem setup and assumptions about density.
ValarDohaeris said:The Attempt at a Solution
I think I may of been too general with the volume in finding [tex]M_0[/tex]
I'm assuming [tex]r_0 = r_M[/tex] although I'm not sure why different notation is used thougj
http://imageshack.us/photo/my-images/3/gravscan.jpg/
That doesn't look quite right. What happened to the constant ro from the density function?ValarDohaeris said:I integrated betwee r0 and 0 and got.
M(r) = 4∏ρ0r30
v2 = GM/r
Not sure where to go from here to get the second term.