By Claudio Vita-Finzi
This good illustrated booklet provides a compact heritage of the sunlight approach from its dusty origins 4,600,000 years in the past to the current day. Its basic goal is to teach how the planets and their satellites, comets, meteors, interplanetary airborne dirt and dust, sunlight radiation and cosmic rays constantly have interaction, occasionally violently, and it displays humanity's development in exploring and analyzing this heritage. The ebook is meant for a basic readership at a time whilst human and robot exploration of house is frequently within the information and may additionally entice scholars in any respect degrees. It covers the necessities yet refers to a wide literature that are accessed through the internet.
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Extra resources for A History of the Solar System
Alfvén H, Arrhenius G (1976) Evolution of the solar system. Asphaug E, Reufer A (2014) Mercury and other iron-rich planetary bodies as relics of inefficient accretion. Bland PA et al (2005) Volartile fractionation in the early solar system and chondrule /matrix complementarity. Boss AP (2003) Rapid formation of outer giant planets by disk instability. Bouvier A, Wadha M (2010) The age of the solar system redefined by the oldest Pb-Pb age of a meteoritic inclusion. Brush SG (1996) Fruitful encounters.
Connelly JN et al (2012) The absolute chronology and thermal processing of solids in the solar protoplanetary disk. dePater I, Lissauer JJ (2001) Planetary sciences. Desch SJ, Morris MA, Connolly HC Jr and Boss AP (2012) The importance of experiments: constraints on chondrule formation models. French B, MacPherson G, Clarke R (1990) Antarctic meteorite teaching collection. Gudipati MS and Yang R (2012) In-situ probing of radiation-induced processing of organics in astrophysical ice analogs – novel laser desorption laser ionization time-of-flight mass spectroscopic studies.
Many of them show evidence of geological activity after their formation, sometimes driven by tidal heating or the consequences of impact. The resulting differentiation is discussed in Chap. 5. The prevailing model has long been that each of the giant planets developed a miniature solar system in its accretion disk, with prograde, near-circular orbits. The capture of passing planetesimals could provide additional satellites with irregular orbits which are prograde or retrograde according to where the capture occurred.
A History of the Solar System by Claudio Vita-Finzi