Answer to Question #88783 in Astronomy | Astrophysics for Navdha

Question #88783
Write down the condition under which a large molecular cloud collapses to give rise
to new stars. Calculate the time of free fall of an HI cloud of density 106 particles/m3
1
Expert's answer
2019-04-30T09:46:39-0400

Write down the condition under which a large molecular cloud collapses to give rise to new stars.

Answer:

For collapse of a cloud with radius R to occur, need either

Mcloud>MJeans=3kTR2GμmHM_{cloud}>M_{Jeans}=\frac{3kTR}{2G \mu m_H}


Calculate the time of free fall of an HI cloud of density 106 particles/m3

Answer:

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×g=G×mMr2(1)m \times g=G \times m \frac{M}{r^2} (1)

The mass M is equal to:


M=4π3×r3×ρ(2)M= \frac{4 \pi}{3}\times r^3 \times ρ (2)

where ρ is the cloud density

We put (2) in (1):


g=4π3G×r×ρ(3)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


g×t22=r(4)\frac{ g \times t^2}{2}=r (4)

We put (3) in (4) and solve for t:


t=32×π×G×ρ(5)t=\sqrt \frac {3}{2\times \pi \times G \times \rho} (5)

The cloud density ρ is equal to:


ρ=n×mH(6)\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: ρ= 1.67 × 10-21 kg/m3

We put the value of cloud density ρ in (5) and get:

t=2× 1015 seconds

One year contains 3× 107 seconds

In this case, t=67.000.000 years


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