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Kelvin-Helmholtz contraction

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Kelvin-Helmholtz contraction [′kel·vən ′helm‚hōlts kən‚trak·shən]
(astrophysics)
A contraction of a star once it is formed and before it is hot enough to ignite its hydrogen; the contraction converts gravitational potential energy into heat, some of which is radiated, with the remainder used to raise the internal temperature of the star.


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