Sediments and sedimentary processes on the Moon and Earth are very different. In the absence of water, an atmosphere, the magnetosphere, and much less oxygen in its rocks, the Moon has neither clay minerals nor carbonates, and no Fe3+. Mechanical weathering by impacts is the principal process of sediment generation on the Moon; on Earth, chemical weathering predominates. Whereas processes of sediment transport are principally ballistic on the Moon, movement by air, water and ice prevail on the Earth. The radical differences between Earth and Moon sediments make them useful end-members between which all sediments of all terrestrial planetary bodies are expected to lie. The purpose of this paper is (l) to compare and contrast major characteristics of the origin, transportation, deposition, and preservation of sediments, especially dust, in the Earth and the Moon, and (2) to suggest how sediments of other rocky planetary bodies, especially Mars, may fit in-between the sediments of the Earth and the Moon.
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Etat : New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. Proceedings of the Conference held in Padova, Italy at the Accademia Galileiana di Scienze Lettere ed Arti, November 8-10, 2000 The Conference on the Earth-Moon relationships brought together a number of distinguished scientists from different f. N° de réf. du vendeur 5830656
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Taschenbuch. Etat : Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -The Conference on the Earth-Moon relationships brought together a number of distinguished scientists from different fields - such as Astronomy, Celestial Mechanics, Chemistry - but also scholars of Literature and Art, to discuss these relationships, their origins, and their influence on human activities and beliefs. 588 pp. Englisch. N° de réf. du vendeur 9789401038553
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Taschenbuch. Etat : Neu. Earth-Moon Relationships | Proceedings of the Conference held in Padova, Italy at the Accademia Galileiana di Scienze Lettere ed Arti, November 8-10, 2000 | Francesca Rampazzi (u. a.) | Taschenbuch | x | Englisch | 2013 | Springer Netherland | EAN 9789401038553 | Verantwortliche Person für die EU: Springer Verlag GmbH, Tiergartenstr. 17, 69121 Heidelberg, juergen[dot]hartmann[at]springer[dot]com | Anbieter: preigu. N° de réf. du vendeur 105580427
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Taschenbuch. Etat : Neu. This item is printed on demand - Print on Demand Titel. Neuware -Sediments and sedimentary processes on the Moon and Earth are very different. In the absence of water, an atmosphere, the magnetosphere, and much less oxygen in its rocks, the Moon has neither clay minerals nor carbonates, and no Fe3+. Mechanical weathering by impacts is the principal process of sediment generation on the Moon; on Earth, chemical weathering predominates. Whereas processes of sediment transport are principally ballistic on the Moon, movement by air, water and ice prevail on the Earth. The radical differences between Earth and Moon sediments make them useful end-members between which all sediments of all terrestrial planetary bodies are expected to lie. The purpose of this paper is (l) to compare and contrast major characteristics of the origin, transportation, deposition, and preservation of sediments, especially dust, in the Earth and the Moon, and (2) to suggest how sediments of other rocky planetary bodies, especially Mars, may fit in-between the sediments of the Earth and the Moon.Springer Verlag GmbH, Tiergartenstr. 17, 69121 Heidelberg 588 pp. Englisch. N° de réf. du vendeur 9789401038553
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Taschenbuch. Etat : Neu. Druck auf Anfrage Neuware - Printed after ordering - Sediments and sedimentary processes on the Moon and Earth are very different. In the absence of water, an atmosphere, the magnetosphere, and much less oxygen in its rocks, the Moon has neither clay minerals nor carbonates, and no Fe3+. Mechanical weathering by impacts is the principal process of sediment generation on the Moon; on Earth, chemical weathering predominates. Whereas processes of sediment transport are principally ballistic on the Moon, movement by air, water and ice prevail on the Earth. The radical differences between Earth and Moon sediments make them useful end-members between which all sediments of all terrestrial planetary bodies are expected to lie. The purpose of this paper is (l) to compare and contrast major characteristics of the origin, transportation, deposition, and preservation of sediments, especially dust, in the Earth and the Moon, and (2) to suggest how sediments of other rocky planetary bodies, especially Mars, may fit in-between the sediments of the Earth and the Moon. N° de réf. du vendeur 9789401038553
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