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Stellar formation
Description:
Star formation. Image 1 of 2. Artwork of a cloud of gas and dust coalescing during the formation of a star. Stars form when gas clouds contract under their own gravity. The gas increases in density and temperature as it contracts, eventually becoming hot enough for nuclear reactions to start. The initial ignition of a new star then blows away much of the surrounding material. Gas clouds rotate as they contract, which flattens the material into a disc. In the surrounding disc of gas and dust, planets and other bodies can form. For an image of this gas cloud at the ignition of a new star, see R590/101.
Credit:
Take 27 Ltd/Science Source
Unique identifier:
SS2175320
Legacy Identifier:
SD5760
Type:
Image
Size:
5315px × 3425px (~52 MB)
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Tags
accretion
astronomy
cloud
contraction
cosmology
disk
dust
embryonic
evolution
forming
gas
gravitational
gravity
horizontal
nebula
planet
planets
primordial
R590/0100
R590/100
R5900100
rotating
Science
solar system
spiral
spiralling
star formation
starbirth
stars
stellar formation
vortex