Zobrazeno 1 - 10
of 19
pro vyhledávání: '"M. Cristina De Sanctis"'
Autor:
M. Cristina De Sanctis, Francesca Altieri, Simone De Angelis, Marco Ferrari, Alessandro Frigeri, sergio Fonte, Eleonora Ammannito, Jeremy Brossier, Marco Giardino, Andrea Apuzzo, nicole costa, lorenzo rossi
Introduction: Mars is a primary destination to search for signs of life and probing the subsurface is a key element in this search. Access to the Martian subsurface, under most altered layers, is needed to understand the nature, timing and duration o
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::0b48e2ba6f648433347feb886fcbe19b
https://doi.org/10.5194/epsc2022-104
https://doi.org/10.5194/epsc2022-104
Autor:
Robert Hodyss, Thomas F. Bristow, Bethany L. Ehlmann, Eleonora Ammannito, Carol A. Raymond, M. Cristina De Sanctis, George R. Rossman
Publikováno v:
Meteoritics & Planetary Science. 53:1884-1901
Mg‐phyllosilicate‐bearing, dark surface materials on the dwarf planet Ceres have NH_4‐bearing materials, indicated by a distinctive 3.06 μm absorption feature. To constrain the identity of the Ceres NH_4‐carrier phase(s), we ammoniated groun
Autor:
Julie Castillo-Rogez, Christopher T. Russell, Joshua P. Emery, M. Cristina De Sanctis, Carle M. Pieters, Carol A. Raymond, Andrew S. Rivkin, Michael J. Toplis, Thomas H. Prettyman, Harry Y. McSween
Publikováno v:
Meteoritics and Planetary Science
Meteoritics and Planetary Science, Wiley, 2018, 53 (9), pp.1793-1804. ⟨10.1111/maps.12947⟩
Meteoritics and Planetary Science, Wiley, 2018, 53 (9), pp.1793-1804. ⟨10.1111/maps.12947⟩
The mineralogy and geochemistry of Ceres, as constrained by Dawn's instruments, are broadly consistent with a carbonaceous chondrite (CM/CI) bulk composition. Differences explainable by Ceres’s more advanced alteration include the formation of Mg-r
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3f1edd044fa67868c51cd2b19c26daf7
https://hal.archives-ouvertes.fr/hal-02410966
https://hal.archives-ouvertes.fr/hal-02410966
Autor:
Oleg Korablev, M. Cristina De Sanctis, Jean-Luc Josset, Håkan Svedhem, Elliot Sefton-Nash, Frances Westall, Ralf Jaumann, Jorge L. Vago, Fred Goesmann, Gerhard Kminek, Fernando Rull, I. G. Mitrofanov, Pietro Baglioni, Andrew J. Coates, Daniel Rodionov, Valérie Ciarletti, ExoMars Team, François Raulin, Jean-Pierre Bibring, William B. Brinckerhoff
The second ExoMars mission will be launched in 2020 to target an ancient landing site interpreted to possess a strong potential for preserving the physical and chemical biosignatures of fossil martian microorganisms, if they existed there. The missio
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ceda1b843895140a1c506aab0b0a8a7b
https://doi.org/10.1016/b978-0-12-809935-3.00011-6
https://doi.org/10.1016/b978-0-12-809935-3.00011-6
Autor:
Abigail C. Allwood, Raymond E. Arvidson, Pietro Baglioni, David Beaty, Luther W. Beegle, Jeff A. Berger, Rohit Bhartia, Jean-Pierre Bibring, Janice L. Bishop, André Brack, William Brinckerhoff, Adrian J. Brown, Nathalie A. Cabrol, Sherry L. Cady, Jeffrey G. Catalano, Valérie Ciarletti, Andrew J. Coates, Alfonso Davila, M. Cristina De Sanctis, Richard C. Elphic, Kenneth A. Farley, Jack D. Farmer, David T. Flannery, Fred Goesmann, Edmond A. Grin, Virginia G. Gulick, Donat-Peter Häder, David Hamilton, Svein-Erik Hamran, Michael H. Hecht, Nancy W. Hinman, Joel A. Hurowitz, Ralf Jaumann, Jean-Luc Josset, Manuel de la Torre Juarez, Gerhard Kminek, Oleg Korablev, Sylvestre Maurice, Alfred S. McEwen, Christopher McKay, Sarah Milkovich, Igor Mitrofanov, Jeffrey Moersch, Nora Noffke, Cynthia Phillips, Richard Quinn, François Raulin, Daniel Rodionov, Jose A. Rodriguez-Manfredi, Fernando Rull, Elliot Sefton-Nash, John R. Skok, Pablo Sobron, Kathryn M. Stack, David Summers, Roger E. Summons, Håkan Svedhem, Luis Teodoro, Jorge L. Vago, Malcolm R. Walter, Kimberley Warren-Rhodes, Frances Westall, David S. Wettergreen, Roger C. Wiens, Kenneth H. Williford, Diane Winter, Pierre Zippi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::04f94ed32ee5cde380f9da1d6495d50e
https://doi.org/10.1016/b978-0-12-809935-3.09992-8
https://doi.org/10.1016/b978-0-12-809935-3.09992-8
Akademický článek
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Autor:
Richard P. Binzel, Harry Y. McSween, Michael J. Gaffey, Vishnu Reddy, L. Le Corre, Andrew W. Beck, Christopher T. Russell, M. Cristina De Sanctis, Carol A. Raymond, Eleonora Ammannito, Thomas B. McCord, Thomas H. Prettyman
Publikováno v:
Meteoritics & Planetary Science. 48:2090-2104
The Dawn mission has provided new evidence strengthening the identification of asteroid Vesta as the parent body of the howardite, eucrite, and diogenite (HED) meteorites. The evidence includes Vesta's petrologic complexity, detailed spectroscopic ch
Autor:
Jessica M. Sunshine, Christopher T. Russell, Carol A. Raymond, M. Teresa Capria, Gianfranco Magni, C. A. Polanskey, Federico Tosi, Sergio Fonte, Andrea Longobardo, M. Cristina De Sanctis, Carle M. Pieters, Francesca Zambon, Harry Y. McSween, Eleonora Ammannito, F. Carraro, Thomas B. McCord, Alessandro Frigeri, Fabrizio Capaccioni, Ernesto Palomba, Lucy A. McFadden, Steven P. Joy, Jean-Philippe Combe, Simone Marchi
Publikováno v:
Meteoritics & Planetary Science. 48:2185-2198
We present global lithological maps of the Vestan surface based on Dawn mission's Visible InfraRed (VIR) Spectrometer acquisitions with a spatial sampling of 200 m. The maps confirm the results obtained with the data set acquired by VIR with a spatia
Autor:
Harry Y. McSween, Federico Tosi, L. Le Corre, Andrew W. Beck, Diego Turrini, Michael J. Toplis, Andreas Nathues, M. Cristina De Sanctis, David W. Mittlefehldt, Eleonora Ammannito, Thomas H. Prettyman, Fabrizio Capaccioni, David P. O'Brien, Christopher T. Russell, Vishnu Reddy, Andrea Longobardo, Carol A. Raymond, Naoyuki Yamashita, Paul M. Schenk, Francesca Zambon, Timothy J. McCoy, Ernesto Palomba
Publikováno v:
Journal of Geophysical Research: Planets. 118:335-346
[1] The estimated excavation depth of the huge Rheasilvia impact basin is nearly twice the likely thickness of the Vestan basaltic crust, so the mantle should be exposed. Spectral mapping by the Dawn spacecraft reveals orthopyroxene-rich materials, s
Publikováno v:
The Astronomical Journal. 133:1836-1846
Thermal evolution models of comet 9P/Tempel 1 have been developed to understand how thermal evolution models of comet nuclei can help to interpret the results of Deep Impact and vice versa, how the Deep Impact results can constrain the comet nuclei m