Zobrazeno 1 - 10
of 19
pro vyhledávání: '"Sabrina Schwinger"'
Publikováno v:
Geophysical Research Letters, Vol 50, Iss 11, Pp n/a-n/a (2023)
Abstract The composition of basaltic melts in equilibrium with the mantle can be determined for several Martian meteorites and in‐situ rover analyses. We use the melting model MAGMARS to reproduce these primary melts and estimate the bulk compositi
Externí odkaz:
https://doaj.org/article/d6c497ebc7884773b52365ad6bfe3fa1
Publikováno v:
Meteoritics & Planetary Science. 57:2143-2157
Autor:
Alessandro Maturilli, Sabrina Schwinger, Enrica Bonato, Maximilian Hamm, Jörn Helbert, Mickael Baque, Giulia Alemanno, Mario D'Amore
Sensitive laboratory instruments on Earth are capable of determining the chemical, isotopic, mineralogical, structural, and physical properties of extraterrestrial samples from the macroscopic level down to the atomic scale, allowing to determine the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::176fd17422e457ffc82642b0c6523f13
https://doi.org/10.5194/epsc2022-489
https://doi.org/10.5194/epsc2022-489
Autor:
Sabrina Schwinger, Nicola Tosi
Publikováno v:
Encyclopedia of Astrobiology ISBN: 9783642278334
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::8a5027aabb8ffe50acf76266ed526f51
https://doi.org/10.1007/978-3-642-27833-4_5606-1
https://doi.org/10.1007/978-3-642-27833-4_5606-1
Introduction During the early stages of lunar evolution, the large amount of heat available from the lunar forming impact led to extensive melting of the Moon’s silicate mantle giving rise to a magma ocean. The fractional crystallization of the lat
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::c421ee03517c1a617f1c036cfe4fa6d8
https://doi.org/10.5194/epsc2021-834
https://doi.org/10.5194/epsc2021-834
Introduction: Laboratory measurements of extra-terrestrial materials like meteorites and ultimately materials from sample return missions can significantly enhance the scientific return of the global remote sensing data. This motivated the addition o
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::82c0f057266eae320056ecfb740bc759
https://doi.org/10.5194/epsc2021-561
https://doi.org/10.5194/epsc2021-561
Autor:
Nikolas Wiesner, Sabrina Schwinger
Introduction: During its early history, the Moon experienced a phase of planetary-scale melting that is commonly referred to as the Lunar Magma Ocean (LMO). Progressive crystallization of the LMO lead to differentiation of the lunar interior into a c
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c1b73f1b26f638734277b0874a03da86
https://doi.org/10.5194/epsc2021-548
https://doi.org/10.5194/epsc2021-548
Publikováno v:
Journal of Geophysical Research: Planets. 124:418-436
The accretion of the debris resulting from the giant collision that formed the Earth‐Moon system caused the formation of a deep lunar magma ocean. The initial composition profile of the Moon results from the solidification of this magma ocean. One