Zobrazeno 1 - 10
of 14
pro vyhledávání: '"Kaveh Pahlevan"'
The deuterium-to-hydrogen (D/H or 2H/1H) ratio of Martian atmospheric water (~6x standard mean ocean water, SMOW) is higher than that of known sources, requiring planetary enrichment. A recent measurement by NASA's Mars Science Laboratory rover Curio
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::575b3cfdae37caacc2a8836c0de24b99
Publikováno v:
Bulletin of the AAS. 53
Publikováno v:
Goldschmidt2021 abstracts.
Publikováno v:
Goldschmidt Abstracts.
Autor:
Jun Wu, Laura Schaefer, Peter R. Buseck, Linda T. Elkins-Tanton, Kaveh Pahlevan, Steven J. Desch
Publikováno v:
Journal of Geophysical Research: Planets. 123:2691-2712
Autor:
Kaveh Pahlevan
Publikováno v:
Nature Geoscience. 11:16-18
Advances in high-precision isotopic analysis have provided key constraints on the origin and early evolution of the Earth and Moon. Measurements of the isotopes of tungsten provide the most stringent constraints on this history.
Autor:
Tomohiro Usui, James P. Greenwood, Kathleen E. Vander Kaaden, Kaveh Pahlevan, Shun-ichiro Karato
Publikováno v:
Space Science Reviews. 214
We review the geochemical observations of water, $\mbox{D}/\mbox{H}$ and volatile element abundances of the inner Solar System bodies, Mercury, Venus, the Moon, and Mars. We focus primarily on the inventories of water in these bodies, but also consid
Autor:
James P. Greenwood, Shun-ichiro Karato, Kathleen E. Vander Kaaden, Kaveh Pahlevan, Tomohiro Usui
Publikováno v:
Space Sciences Series of ISSI ISBN: 9789402416275
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::191997169bab33c46ff2ea9de4259451
https://doi.org/10.1007/978-94-024-1628-2_5
https://doi.org/10.1007/978-94-024-1628-2_5
Publikováno v:
Earth Planet Sci Lett
The Moon-forming giant impact extensively melts and partially vaporizes the silicate Earth and delivers a substantial mass of metal to Earth's core. Subsequent evolution of the magma ocean and overlying atmosphere has been described by theoretical mo
Autor:
Alessandro Morbidelli, Kaveh Pahlevan
Publikováno v:
Nature. 527:492-494
The Moon is generally thought to have formed from the debris ejected by the impact of a planet-sized object with the proto-Earth towards the end of planetary accretion. Modeling of the impact process predicts that the lunar material was disaggregated