By Claudio Vita-Finzi

ISBN-10: 331933848X

ISBN-13: 9783319338484

ISBN-10: 3319338501

ISBN-13: 9783319338507

This good illustrated ebook offers a compact historical past of the sunlight procedure from its dusty origins 4,600,000 years in the past to the current day. Its basic target is to teach how the planets and their satellites, comets, meteors, interplanetary airborne dirt and dust, sun radiation and cosmic rays continuously engage, occasionally violently, and it displays humanity's growth in exploring and analyzing this heritage. The booklet is meant for a normal readership at a time whilst human and robot exploration of area is frequently 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 info for A History of the Solar System

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Kokubo E, Ida S (2012) Dynamics and accretion of planetesimals. Prog Theor Exper Phys. Lewis JS (1995) Physics and chemistry of the solar system (rev ed). Lissauer JJ (2006) Planet formation, protoplanetary disks and debris disks. Lissauer JJ, Stevenson DJ (2007) Formation of giant planets. 23 billion years ago. Lowell P (1903) The solar system. Lynch P (2003) On the significance of the Titius-Bode law for the distribution of the planets. Marzari F et al (2002) Origin and evolution of Trojan Asteroids.

Morbidelli A et al (2005) Chaotic capture of Jupiter’s Trojan asteroids in thre early solar syste,. Norman MD, Duncan RA, Huard JJ (2006) Identifying impact events within the lunar cataclysm from 40Ar-39Ar ages and compositions of Apollo 16 impact melt rocks. Perets HB, Kouwenhoven MBN (2012) On the origin of planets at very wide orbits from the recapture of free floating planets. Astrophys J 750: 83. Roche E (1849) La figure d’une masse fluide soumise à l’attraction d’un point éloigné. See TJJ (1910) Researches on the evolution of the stellar systems II.

5 Gyr ago would have been more massive by a mere 1/10,000 of the present value. Indeed, although the Sun loses 109 tonnes/sec, direct measurement by the Michelson Doppler Imaging instrument on the SOHO satellite of solar diameter over much of a solar cycle has found no evidence that annual diameter change exceeds 15 mas (milliarcsecond or 1/1000 of a second of arc) [11]. Of course mass loss may have been greater in the past especially if the Sun experienced a spell as a T tauri star. As it happens, the presence of neon-21 (21Ne) in a number of carbonaceous chondrites (including the Murchison meteorite) indicates irradiation by energetic protons from the young Sun.

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A History of the Solar System by Claudio Vita-Finzi


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