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The
Solar Nebula
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The solar system formed from
a clump of gas
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There was enough gas to self
gravitate
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As gas clump contracted,
it got hotter
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Gas at center got hottest
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Analogy: lecture hall in
summer
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became protosun
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Gas doesn't all head perfectly
to center
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As gas contracts, spins faster
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Conservation of angular momentum
(ice skater illustration)
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Spinning faster causes disk
shape
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We see stars forming in other
nebulae
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Disks called protoplanetary
disks (proplyds)
Orion Nebula
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