Zobrazeno 1 - 10
of 34
pro vyhledávání: '"B. Bultel"'
Autor:
B. Bultel, S. C. Werner
Publikováno v:
The Planetary Science Journal, Vol 4, Iss 8, p 146 (2023)
Studying the geology of a terrestrial body and its evolution requires being able to set up a chronology. Crater statistics is a powerful tool to do so. However, calibration of this method, which is derived on the Moon, requires properly defined geolo
Externí odkaz:
https://doaj.org/article/13f02859dd5e4ea18c1a8b8c98de1107
Autor:
Francois Poulet, Håkon O. Austrheim, Elise M. Harrington, Agata M. Krzesińska, Cateline Lantz, Damien Loizeau, Jean-Christophe Viennet, Stephanie C. Werner, B. Bultel, Henning Dypvik
Serpentinization and carbonation have affected ultramafic rocks on Noachian Mars in several places called here serpentinization-carbonation systems (SCS). Among the most prominent SCS revealing mineral assemblages characteristic of serpentinization/c
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::90cb37d3b1587348957d2c350c1e78c7
https://doi.org/10.5194/epsc2021-230
https://doi.org/10.5194/epsc2021-230
Autor:
D. Loizeau, Stephanie C. Werner, David Craw, Richard H. April, François Poulet, Agata M. Krzesińska, B. Bultel
In 2022, ESA/ROSCOSMOS will launch the ExoMars2022 rover mission to Mars. The selected landing site for the mission is Oxia Planum, a wide, Noachian-age, phyllosilicate-bearing plain located on the SE border of Chryse Planitia. The Fe,Mg-rich clay mi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::787177db71de86b179d20947b5ba5762
https://doi.org/10.5194/egusphere-egu21-841
https://doi.org/10.5194/egusphere-egu21-841
Autor:
David Craw, Damien Loizeau, Richard H. April, Stephanie C. Werner, Francois Poulet, Agata M. Krzesińska, B. Bultel
Publikováno v:
Astrobiology
Oxia Planum is a Noachian plain on Mars. It was chosen as the final landing site for in situ studies by ExoMars 2022 rover. The main scientific objectives of the mission are to understand the mineralogy and aqueous evolution of ancient Mars with rele
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0235842d5d77190761a56edfaf053f23
http://hdl.handle.net/10852/88753
http://hdl.handle.net/10852/88753
Autor:
Francois Poulet, Marco Veneranda, Helge Hellevang, Fernando Rull, Henning Dypvik, Agnes Cousin, Jean-Christophe Viennet, Dwijesh Ray, C. Saetre, B. Bultel, Agata M. Krzesińska, Damien Loizeau, Stephanie C. Werner
Publikováno v:
Planetary and Space Science
Planetary and Space Science, 2021, 208, ⟨10.1016/j.pss.2021.105339⟩
Planetary and Space Science, 2021, 208, ⟨10.1016/j.pss.2021.105339⟩
International audience; The Planetary Terrestrial Analogues Library (PTAL) is a dedicated lithological collection that currently consists of 102 terrestrial rock samples selected to be possible Mars analogues. The ultimate goal is improving future re
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bea538a87dad6149d019cd283155707d
http://hdl.handle.net/10852/89930
http://hdl.handle.net/10852/89930
In 2020, ESA/ROSCOSMOS will launch ExoMars2020 rover mission to Mars. The selected landing site for the mission is Oxia Planum, a wide Noachian-aged clay mineral-bearing plain. The Fe,Mg-rich clay mineral deposits in Oxia are one of the largest expos
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::04005147dd1dc4f3f1b6e0bf8eba9b48
https://doi.org/10.5194/egusphere-egu2020-10649
https://doi.org/10.5194/egusphere-egu2020-10649
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Publikováno v:
Journal of Geophysical Research: Planets. 122:2328-2343
Publikováno v:
Chemical Geology
Chemical Geology, Elsevier, 2019, ⟨10.1016/j.chemgeo.2019.07.009⟩
Chemical Geology, 2019, ⟨10.1016/j.chemgeo.2019.07.009⟩
Chemical Geology, Elsevier, 2019, ⟨10.1016/j.chemgeo.2019.07.009⟩
Chemical Geology, 2019, ⟨10.1016/j.chemgeo.2019.07.009⟩
On Mars, mineral sequences have been detected and they are composed of a top layer of Al-rich clay minerals, then (Al, Fe)-rich clay minerals and a bottom layer composed of (Mg, Fe)-rich clay minerals. By analogy with Earth, such sequences are interp
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::09851487e9d8b6e6fbe93c00b6ed927e
https://hal.archives-ouvertes.fr/hal-03127691
https://hal.archives-ouvertes.fr/hal-03127691