Earth-Moon Relationships: Proceedings of the Conference held in Padova, Italy at the Accademia Galileiana di Scienze Lettere ed Arti, November 8–10, 2000Cesare Barbieri, Francesca Rampazzi Springer Science & Business Media, 29.06.2013 - 575 Seiten 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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... crustal evolution . Be- cause the lunar surface is completely covered by regolith , and no bedrock has been directly observed or sampled , sediment is the principal guide to the lunar crust , past and present . Provenance analysis of ...
... crustal evolution . Be- cause the lunar surface is completely covered by regolith , and no bedrock has been directly observed or sampled , sediment is the principal guide to the lunar crust , past and present . Provenance analysis of ...
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... crustal rocks of the body . Much of this is due to the fact that remotely sensed signals integrate over a limited depth from the surface . For example , on the Moon , y - rays may integrate to a depth of about 50 cm , the reflectance of ...
... crustal rocks of the body . Much of this is due to the fact that remotely sensed signals integrate over a limited depth from the surface . For example , on the Moon , y - rays may integrate to a depth of about 50 cm , the reflectance of ...
Seite 149
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Inhalt
24 | |
45 | |
R BENN The Moon and the Origin of Life 6166 | 61 |
Claire de Lune on the Italian Space | 85 |
GUY CONSOLMAGNO SJ Apollo Samples and the Geochemical | 114 |
MARK DEANTONIO Lunacy in Mentally Disturbed Children 129131 | 133 |
JAMES W HEAD III Lunar and Planetary Perspectives on | 153 |
Andere Ausgaben - Alle anzeigen
Earth-Moon Relationships: Proceedings of the Conference held in Padova ... Cesare Barbieri,Francesca Rampazzi Eingeschränkte Leseprobe - 2001 |
Earth-Moon Relationships: Proceedings of the Conference held in Padova ... Cesare Barbieri,Francesca Rampazzi Keine Leseprobe verfügbar - 2013 |
Häufige Begriffe und Wortgruppen
2001 Kluwer Academic abundances activity anorthositic Apollo Apollo 15 asteroids astronomical Basin breccias Carlini and Plana century changes chemical chondrites Clementine composition cosmic rays Cosmochim crust crustal D-CIXS dust Earth eclipse effects elements evolution Figure full Moon Galileo Geochim geological Geophys global HED meteorites ICEUM4 impact craters influence Italy Kluwer Academic Publishers KREEP Laplace light Luna lunar atmosphere lunar craters lunar cycle lunar map lunar meteorite lunar phase Lunar Prospector lunar surface LUNEX mantle mare basalts Mars measurements melt meteor meteorites Moon and Planets Moon phases Moon's moonlight movie Naylor nitrogen observations Observatory orbit origin Palolo palolo worm period plate tectonics regolith reproduction rhythms rocks samples satellite Science scientific sediments semilunar shows SMART-1 solar system solar wind South Pole-Aitken Basin space spacecraft spawning spectrometer stars studies telescope temperature terrestrial theory tidal tides University of Padova variations volcanic X-ray