Download A History of the Solar System by Claudio Vita-Finzi PDF

By Claudio Vita-Finzi

This good illustrated e-book offers a compact historical past of the sun process from its dusty origins 4,600,000 years in the past to the current day. Its fundamental objective is to teach how the planets and their satellites, comets, meteors, interplanetary dirt, sun radiation and cosmic rays constantly engage, occasionally violently, and it displays humanity's development in exploring and examining this background. The e-book is meant for a basic readership at a time whilst human and robot exploration of house is usually within the information and will additionally entice scholars in any respect degrees. It covers the necessities yet refers to a wide literature which are accessed through the internet.

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Additional resources for A History of the Solar System

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Wark DA (1978) Birth of the presolar nebula: the sequence of condensation revealed in the Allende meteorite. Wasserburg GJ (1995) Solar models with helium and heavy-element diffusion. Wiechert U et al (2001) Oxygen isotopes and the moon-forming giant impact. Williams JP, Cieza LA (2010) Protoplanetary disks and their evolution. Wood JA (1986) Moon over Mauna Loa. Woolfson MM (2011) On the origin of planets. Zhang Y (1998) The young age of Earth. Geochim Cosmochim Acta 62: 3185-3189 Chapter 4 The Solar Nucleus Abstract The Sun, which embodies much of the mass of our solar system, has evolved substantially since its coagulation from the nebula.

5 Myr will have been converted into planetesimals or planets, accreted onto the star or dumped from the system [39]. Whatever one’s views about the hetegonic thesis, some kind of accretion is evidently central to most accounts of solar system origins [11]. Calculations based on plausible dust density in a turbulent medium and on the assumption that all collisions result in sticking—perhaps through magnetic, mechanical or electrostatic forces or through partial fusion through impact—suggest that after 4000 yr particles with a mass of 10 g might be common and that after 10,000 yr much of the dust might form part of bodies some of them measuring thousands of kilometers [24] and qualifying as protoplanets.

The capture theory of cosmical evolution. Showalter MR, Hedman MM, Bjurns JA (2011) The impact of Comet Shoemaker-Levy-9 sends ripples through the rings of Jupiter. Spohn T, Johnson T, Breuer D (eds) (2014) Encyclopedia of the solar system (3rd ed). Van der Marel N, et al (2015) Resolved gas cavities in transitional disks inferred from CO isotopologs with ALMA. Astr Astrophys 585: A58. Wark DA (1978) Birth of the presolar nebula: the sequence of condensation revealed in the Allende meteorite.

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