A cloud wtith radius R, mass M, and temperature T will collapse to form a star if the total energy of the cloud is <0, i.e, if the (absolute value) of the potential energy exceeds the thermal energy of the cloud:
We can rewriter (1) as
"\\frac {3}{5} \\frac {GM^2}{R}=N \\frac {3}{2} kT (2)"
where N is total number of particles in cloud
The total number of particles in cloud is can written as
Solving for R gives:
Using (4) we get:
R=7×108 m
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