The origin of the Earth.
It is not possible to consider the formation of the Earth in isolation without reference to the formation of the rest of the solar system. A brief account is given of the current scientific consensus on that topic, explaining the origin of an inner solar system rocky planet depleted in most of the gaseous and icy components of the original solar nebula. Volatile element depletion occurred at a very early stage in the nebula, and was probably responsible for the formation of Jupiter before that of the inner planets. The Earth formed subsequently from accumulation of a hierarchy of planetesimals. Evidence of these remains in the ancient cratered surfaces and the obliquities (tilts) of most planets. Earth melting occurred during this process, as well as from the giant Moon-forming impact. The strange density and chemistry of the Moon are consistent with an origin from the mantle of the impactor. Core-mantle separation on the Earth was coeval with accretion. Some speculations are given on the origin of the hydrosphere.
Taylor
S R
SR
Department of Nuclear Physics, Australian National University, Canberra, Australia.
D001272:Atmosphere; D018534:Earth, Planet; D019419:Evolution, Planetary; D005118:Extraterrestrial Environment; D019110:Meteoroids; D018543:Minor Planets; D016081:Moon; D005741:Noble Gases / Q000737:chemistry; D016083:Planets; D011188:Potassium; D012413:Rubidium; D016082:Solar System; D013324:Strontium; D014501:Uranium; D014867:Water
D005741:Noble Gases; D014867:Water; D014501:Uranium; D012413:Rubidium; D011188:Potassium; D013324:Strontium