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, 30 sept. 2001 - 575 pagini 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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... Prospector Missions 253-269 MICHAEL MENDILLO / The Atmosphere of the Moon 271-277 ELFED MORGAN / The Moon and Life on Earth 279-290 E. NAYLOR / Marine Animal Behaviour in Relation to Lunar ... Moon 411-418 JEAN - PIERRE SWINGS / " Earth - ...
... Prospector Missions 253-269 MICHAEL MENDILLO / The Atmosphere of the Moon 271-277 ELFED MORGAN / The Moon and Life on Earth 279-290 E. NAYLOR / Marine Animal Behaviour in Relation to Lunar ... Moon 411-418 JEAN - PIERRE SWINGS / " Earth - ...
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Cuprins
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II | 5 |
III | 25 |
IV | 45 |
V | 51 |
VI | 61 |
VII | 67 |
IX | 85 |
XXXIV | 363 |
XXXV | 365 |
XXXVI | 379 |
XXXVII | 391 |
XXXIX | 405 |
XL | 411 |
XLI | 419 |
XLII | 427 |
X | 87 |
XI | 99 |
XII | 115 |
XIII | 127 |
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XIX | 179 |
XX | 201 |
XXI | 209 |
XXIV | 225 |
XXV | 237 |
XXVI | 245 |
XXVII | 253 |
XXVIII | 271 |
XXIX | 279 |
XXX | 291 |
XXXI | 303 |
XXXII | 343 |
XXXIII | 351 |
XLIII | 443 |
XLIV | 445 |
XLV | 453 |
XLVI | 463 |
XLVIII | 479 |
XLIX | 487 |
L | 497 |
LI | 499 |
LII | 505 |
LIII | 515 |
LIV | 517 |
LV | 523 |
LVI | 533 |
LVII | 539 |
LVIII | 545 |
LIX | 547 |
LX | 557 |
LXI | 561 |
LXII | 567 |
LXIII | 573 |
Alte ediții - Afișează-le pe toate
Earth-Moon Relationships: Proceedings of the Conference held in Padova ... Cesare Barbieri,Francesca Rampazzi Previzualizare limitată - 2013 |
Earth-Moon Relationships: Proceedings of the Conference held in Padova ... Cesare Barbieri,Francesca Rampazzi Nu există previzualizare disponibilă - 2013 |
Earth-Moon Relationships Cesare Barbieri,Francesca Rampazzi Nu există previzualizare disponibilă - 2014 |
Termeni și expresii frecvente
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 Earth-Moon eclipse effects elements evolution Figure full Moon Galileo geological Geophys global HED meteorites ICEUM4 impact 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 Netherlands nitrogen observations Observatory orbit origin 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