Alfie114
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- TL;DR
- I have a question about the virial theorem as applied to a cluster of stars.
Anyone able to help if I provide you with more details?
The discussion revolves around the application of the Virial Theorem to a star cluster system composed of stars and gas. Participants are exploring how to calculate the kinetic energy of the system under specific conditions, including assumptions about mass distribution and equilibrium.
The discussion remains unresolved, with no consensus on the approach to calculating kinetic energy or the specific equations to use.
Participants have not fully defined all variables or assumptions, and there may be dependencies on specific definitions of terms like kinetic energy and potential energy.

You need to use math latex notation. Its hard to understand your equations like this.Alfie114 said:OK we have a star cluster (the system) which is made up from stars (total mass M sub *) and gas (total mass M sub g). The stars and gas are all distributed as spheres of constant density and a finite radius r sub c.
The total mass of the stars and the gas is different but we can assume that M sub g = f*M sub *
If the system is unrotating and in equilibrium how do we calculate the kinetic energy in terms of r sub c, f and M sub *?
We can take 2KE + PE = 0 where KE = (-3/5) (GM^2/R) and PE = (3kT/2)*n where n is the total number of particles = (M/mu*m sub H) where mu=1 and m sub H is the mass of a hydrogen atom.