For collapse of a cloud with radius R to occur, need either
"M_{cloud} \\gt M_{Jeans}=\\frac{3kTR}{2G \\mu m_H}"
The acceleration g felt by a test particle for a spherically symmetric distribution of mass M and radius r.
From Newton's second law, the equation of motion for a test particle at the edge of the cloud is then
"m \\times g=G \\times m \\frac{M}{r^2} (1)"
The mass M is equal to:
"M= \\frac{4 \\pi}{3}\\times r^3 \\times \u03c1 (2)"
We put (2) in (1):
"g=\\frac{4 \\pi}{3}G \\times r \\times \\rho (3)"
If it starts initially at rest, then (if acceleration is constant) it will reach the center when
"\\frac{ g \\times t^2}{2}=r (4)"
We put (3) in (4) and solve for t:
"t=\\sqrt \\frac {3}{2\\times \\pi \\times G \\times \\rho} (5)"
The cloud density ρ is equal to:
"\\rho=n \\times m_H (6)"
where n=106 particles/m3 ; mH = 1.67 × 10-27 kg
Using (6) we calculate the value of cloud density ρ: "\u03c1= 1.67 \u00d7 10^{-21} kg\/m3"
We put the value of cloud density ρ in (5) and get: "t = 2\u00d7 10^{15} seconds"
One year contains 3× 107 seconds
So we get, t=67.000.000 years
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