Zobrazeno 1 - 10
of 16
pro vyhledávání: '"Adrien Morison"'
The flyby of Pluto by the New Horizons spacecraft in 2015 revealed stricking features in a nitogen ice filled basin named Sputnik Planitia (SP). On the large (few 10 km) scale, irregular polygons [1] have been interpreted as resulting from solid-stat
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::a423571080fec166363e25c443d28493
https://doi.org/10.5194/epsc2022-434
https://doi.org/10.5194/epsc2022-434
Study of convection in high-pressure ice layers of large icy moons and implications for habitability
The existence of a high-pressure (HP) ice layer between the silicate core and the liquid ocean in large icy moons and ocean worlds is usually seen as a barrier to habitability, preventing a direct contact and therefore transfer of nutrients from the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::a713e92280e82afffa4ce7a4b7a623d3
https://doi.org/10.5194/epsc2022-650
https://doi.org/10.5194/epsc2022-650
Publikováno v:
Nature
Nature, 2021, 600, pp.419-423. ⟨10.1038/s41586-021-04095-w⟩
Nature, 2021, 600, pp.419-423. ⟨10.1038/s41586-021-04095-w⟩
International audience; Sputnik Planitia is a nitrogen-ice-filled basin on Pluto1. Its polygonal surface patterns2 have been previously explained as a result of solid-state convection with either an imposed heat flow3 or a temperature difference with
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::99d1163d4228ec426dfea7034f53660f
https://pubmed.ncbi.nlm.nih.gov/34912087
https://pubmed.ncbi.nlm.nih.gov/34912087
Autor:
Adrien Morison, Antoine Rozel, Daniela Bolrão, Stéphane Labrosse, Maxim D. Ballmer, Paul J. Tackley, Renaud Deguen, Thierry Alboussière
The early evolution of the Earth was likely affected by a large scale magma ocean, in particular in the aftermath of the giant impact that formed the Moon. The exact structure and dynamics of the Earth following that event is unknown but several poss
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::72cf0f8e7548d947852dd2ffd1923f26
https://doi.org/10.5194/egusphere-egu21-8013
https://doi.org/10.5194/egusphere-egu21-8013
Autor:
Paul J. Tackley, Daniela Bolrão, Adrien Morison, Antoine Rozel, Stéphane Labrosse, Maxim D. Ballmer, Thierry Alboussière, Renaud Deguen
The light plagioclase-enriched crust as well as the KREEP layer at the surface of the Moon are believed to be remnants of the bottom-up crystallization of a global Lunar Magma Ocean. In such a setup, the primitive Lunar solid mantle is coated by a li
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::31782a8ed2363ed72587f99a235d5913
https://doi.org/10.5194/egusphere-egu21-6258
https://doi.org/10.5194/egusphere-egu21-6258
The existence of a high pressure ice layer between the silicate core and the liquid ocean in large icy moons and ocean worlds is usually seen as a barrier to habitability, preventing the compounds needed for life to flow into the ocean. More recently
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::aabe01ee0e7663923ae3ea51f95c32f7
https://doi.org/10.5194/egusphere-egu21-12691
https://doi.org/10.5194/egusphere-egu21-12691
Autor:
Kenny Vilella, Maxim D. Ballmer, Adrien Morison, Rob Spaargaren, Daniela Bolrão, Ananya Mallik, Miki Nakajima
Publikováno v:
Goldschmidt2021 abstracts.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::89011b2e43f8830690fffdb2666bf2dc
https://doi.org/10.7185/gold2021.4839
https://doi.org/10.7185/gold2021.4839
Autor:
Daniela Paz Bolrão, Maxim Dionys Ballmer, Adrien Morison, Antoine Billy Rozel, Patrick Sanan, Stéphane Labrosse, Paul James Tackley
After accretion and formation, terrestrial planets go through at least one magma ocean episode. As the magma ocean crystallises, it creates the first layer of solid rocky mantle. Two different scenarios of magma ocean crystallisation involve that the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::739cb5638bd11f976d4efdd246fc3a6a
https://doi.org/10.5194/se-2020-49
https://doi.org/10.5194/se-2020-49
Autor:
Antoine Rozel, Daniela Bolrão, Paul J. Tackley, Stéphane Labrosse, Maxim D. Ballmer, Adrien Morison
Several studies suggest that Mars went through an episode of Magma Ocean (MO) early in its history. When the MO crystallises, solid mantle appears. The crystallisation of this MO starts at the Core-Mantle Boundary (CMB) and continues upwards to the s
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::628a8be52baa17f86e370e786fb48774
https://doi.org/10.5194/egusphere-egu2020-5357
https://doi.org/10.5194/egusphere-egu2020-5357
Autor:
Adrien Morison, Rob Spaargaren, Miki Nakajima, Ananya Mallik, Daniela Bolrão, Maxim D. Ballmer
Terrestrial planets evolve through various stages of large-scale melting, or magma oceans, due to the energy release during accretion and differentiation. Any magma ocean is thought to become progressively enriched in FeO and incompatible elements up
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::01591443e49a02588dfe152aeebaefc6
https://doi.org/10.5194/egusphere-egu2020-11800
https://doi.org/10.5194/egusphere-egu2020-11800