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Autor:
Sanjeev Gupta, Nicolas Mangold, Bell, Jim F., Olivier Gasnault, Tarnas, J. D., Sholes, S., Briony Horgan, Cathy Quantin-Nataf, Brown, A., Stéphane Le Mouélic, Roberta Yingst, Olivier Beyssac, Bosak, T., Fred Calef, Gwénaël CARAVACA, Ehlmann, B., Kenneth Farley, Grotzinger, John P., Hickman-Lewis, K., Holm-Alwmark, S., Kah, Linda C., Kanine, M., Martinez-Frias, J., Mclennan, Scott M., Sylvestre Maurice, Nuñez, J., Ollila, A. M., Gerhard Paar, Paolo Pilleri, Rice, J., Rice, M., Simon, J., Shuster, D., Katie Stack‐morgan, Vivian Sun, Treiman, Allan H., Weiss, B., Wiens, Roger C., Williams, A., Williams, N., Williford, Kenneth H.
Publikováno v:
53rd Lunar and Planetary Science Conference
Lunar and Planetary Science Conference
Lunar and Planetary Science Conference, Lunar and Planetary Institute, Mar 2022, The Woodlands, United States. pp.2295
HAL
Lunar and Planetary Science Conference
Lunar and Planetary Science Conference, Lunar and Planetary Institute, Mar 2022, The Woodlands, United States. pp.2295
HAL
International audience; Orbital and rover observations of relictgeomorphic features and stratigraphic architectures indicate Mars once had a warmer, wetter climate. Constraining the character, relative timing and persistence of ancient aqueous activi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::f07e17f8cff6e90439f366753b7dc9df
https://hal.science/hal-03594054/document
https://hal.science/hal-03594054/document