Books > Science & Mathematics > Astronomy, space & time > Galaxies, clusters, intergalactic matter
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Accretion of Extraterrestrial Matter Throughout Earth's History (Hardcover, 2001 ed.)
Loot Price: R3,079
Discovery Miles 30 790
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Accretion of Extraterrestrial Matter Throughout Earth's History (Hardcover, 2001 ed.)
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Every year Earth is bombarded with about 40,000 tons of
extraterrestrial material. This includes microscopic cosmic dust
particles shed by comets and asteroids in outer space, meteorites,
as well as large comets and asteroids that have led to catastrophic
events in the geologic past. Originally considered only a
curiosity, extraterrestrial matter found on Earth provides the only
samples we have from comets, asteroids and other planets. Only
recently mankind has started to actively collect extraterrestrial
matter in space (Apollo program, Stardust mission) rather than to
wait for its delivery to Earth. Still, most of our knowledge of the
origin and evolution of our solar system is based on careful
studies of meteorites, cosmic dust, and traces of large impact
events in the geologic record such as the mass extinction that
terminated the Cretaceous Period and led to the extinction of the
dinosaurs. This book summarizes our current knowledge of the
properties, origin, orbital evolution and accretion mechanism of
extraterrestrial matter accreted on Earth and sheds light on
accretion processes and fluxes in the geologic past. The chapters
in the first part of the book are arranged in order to follow
extraterrestrial matter from its origin in space, its orbital
evolution on its way to Earth, its interaction with the Earth
magnetosphere and atmosphere to its more or less violent collision
with the Earth's surface. In the second part of the book several
chapters deal with the present?day flux of cosmic dust and
meteorites to Earth. Finally, several chapters deal with the
reconstruction of the accretion history of extraterrestrial matter
on Earth, starting with the most recent geologic past and ending
with the very early, violent accretion period shortly after the
formation of Earth, Moon and other solid planets in our solar
system.
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