Solar Evolution

Details Solar Evolution Solar Evolution

Nov 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000eaa..booke1981.&link_type=abstract

"Encyclopedia of Astronomy and Astrophysics, Edited by Paul Murdin, article 1981. Bristol: Institute of Physics Publishing, 2001

Astronomy and Astrophysics

Astrophysics

Sun, Basic Solar Properties

Scientific paper

It is generally accepted that the formation of the Sun arose from the passage of a shock wave through an interstellar cloud (see, for example, INTERSTELLAR MATTER), causing part of the cloud to become gravitationally bound. The major component of the cloud was hydrogen, together with about 25% helium, and more massive elements in minor proportions....

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