4. Building of a Habitable Planet

被引:0
|
作者
Hervé Martin
Francis Albarède
Philippe Claeys
Muriel Gargaud
Bernard Marty
Alessandro Morbidelli
Daniele L. Pinti
机构
[1] Université Blaise Pascal,Laboratoire Magmas et Volcans
[2] Ecole Normale Supérieure,DGLG
[3] Vrije Universiteit Brussel,WE
[4] Université Bordeaux 1,Observatoire Aquitain des Sciences de l’Univers
[5] Ecole Nationale Supérieure de Géologie,GEOTOP
[6] Observatoire de la Côte d’Azur,UQAM
[7] Université du Québec à Montréal,McGill
来源
Earth, Moon, and Planets | 2006年 / 98卷
关键词
Hadean; Archaean; continental growth; atmosphere and ocean formation; Late Heavy Bombardment;
D O I
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中图分类号
学科分类号
摘要
Except the old Jack Hills zircon crystals, it does not exit direct record of the first 500 Ma of the Earth history. Consequently, the succession of events that took place during this period is only indirectly known through geochemistry, comparison with other telluric planets, and numerical modelling. Just after planetary accretion several episodes were necessary in order to make life apparition and development possible and to make the Earth surface habitable. Among these stages are: the core differentiation, the formation of a magma ocean, the apparition of the first atmosphere, oceans and continents as well as the development of magnetic field and of plate tectonics. In the same time, Earth has been subject to extraterrestrial events such as the Late Heavy Bombardment (LHB) between 3.95 and 3.8 Ga. Since 4.4–4.3 Ga, the conditions for pre-biotic chemistry and appearance of life were already met (liquid water, continental crust, no strong meteoritic bombardment, etc...). This does not mean that life existed as early, but this demonstrates that all necessary conditions assumed for life development were already present on Earth.
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页码:97 / 151
页数:54
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