Zobrazeno 1 - 10
of 239
pro vyhledávání: '"M. C. De Sanctis"'
Autor:
M. Formisano, F. Altieri, A. Frigeri, M. C. De Sanctis, C. Federico, G. Magni, E. Ammannito, S. De Angelis, M. Ferrari
Publikováno v:
Advances in Astronomy, Vol 2023 (2023)
The aim of this work is to characterize, from a thermophysical perspective, the dark resistant unit (DRU) characterizing Germania Lacus in the Oxia Planum Region, providing new insights to constrain the nature of the materials which compose this unit
Externí odkaz:
https://doaj.org/article/65b2d390ebf5411daabcee5fe004c2b1
Autor:
M. Formisano, M. C. De Sanctis, C. Federico, G. Magni, F. Altieri, E. Ammannito, S. De Angelis, M. Ferrari, A. Frigeri
Publikováno v:
Advances in Astronomy, Vol 2021 (2021)
Numerical simulations are required to thermophysically characterize Oxia Planum, the landing site of the mission ExoMars 2022. A drilling system is installed on the ExoMars rover, and it will be able to analyze down to 2 meters in the subsurface of M
Externí odkaz:
https://doaj.org/article/b04f67e085234c3eb0305e72e2652db7
Autor:
S. Marchi, A. I. Ermakov, C. A. Raymond, R. R. Fu, D. P. O’Brien, M. T. Bland, E. Ammannito, M. C. De Sanctis, T. Bowling, P. Schenk, J. E. C. Scully, D. L. Buczkowski, D. A. Williams, H. Hiesinger, C. T. Russell
Publikováno v:
Nature Communications, Vol 7, Iss 1, Pp 1-9 (2016)
Studying craters on atmosphere-less bodies can unlock information about planetesimal histories. Here, Marchi et al. present results from the NASA Dawn mission to Ceres showing that craters >100–150 km in size are largely absent, and find that Ceres
Externí odkaz:
https://doaj.org/article/08289b965cc44a4ca994d234732687ce
Autor:
Gianfranco Magni, M. Ferrari, Costanzo Federico, Francesca Altieri, Alessandro Frigeri, M. C. De Sanctis, Eleonora Ammannito, Michelangelo Formisano, S. De Angelis
Publikováno v:
Advances in Astronomy, Vol 2021 (2021)
Numerical simulations are required to thermophysically characterize Oxia Planum, the landing site of the mission ExoMars 2022. A drilling system is installed on the ExoMars rover, and it will be able to analyze down to 2 meters in the subsurface of M
Autor:
M. C. De Sanctis, Federico Tosi, David P. O'Brien, Christopher T. Russell, Julie Castillo-Rogez, Hanna G. Sizemore, Jennifer E.C. Scully, Simone Marchi, Paul M. Schenk, Andreas Nathues, Carol A. Raymond, Britney E. Schmidt, C. M. Pieters, Dewight Williams, Debra Buczkowski, Adrian Neesemann
Publikováno v:
Nature Communications, Vol 11, Iss 1, Pp 1-11 (2020)
Nature Communications
Nature Communications
Hydrothermal processes in impact environments on water-rich bodies such as Mars and Earth are relevant to the origins of life. Dawn mapping of dwarf planet (1) Ceres has identified similar deposits within Occator crater. Here we show using Dawn high-
Autor:
Michelangelo Formisano, Julie Castillo-Rogez, M. C. De Sanctis, Gianfranco Magni, Costanzo Federico
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 494:5704-5712
Ceres is the largest body in the Main Belt, and it is characterized by a large abundance of water ice in its interior. This feature is suggested by its relatively low bulk density (2162 kg m−3), while its partial differentiation into a rocky core a
Autor:
S. De Angelis, M. C. De Sanctis, F. Altieri, M. Ferrari, E. Ammannito, S. Novi, M. Dami, A. Barbis, F. Antonacci, F. Villa, F. Ruggiero, S. Fonte, M. Formisano, P. Tinivelli, M. Giardino, R. Mugnuolo, S. Pirrotta
Publikováno v:
Review of Scientific Instruments. 93:123704
The Ma_MISS spectrometer is integrated within the drilling system of the Rosalind Franklin ExoMars rover. This paper reports the on-ground calibration campaign performed on the spectrometer. Here, we focus on the spectral calibration of the instrumen
Autor:
Federico Tosi, S. Fonte, C. T. Russel, M. C. De Sanctis, Filippo Giacomo Carrozzo, Batiste Rousseau, Carol A. Raymond, Mauro Ciarniello, Eleonora Ammannito, P. Scarica, Andrea Raponi, Alessandro Frigeri
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 653 (A118), pp.23. ⟨10.1051/0004-6361/202141503⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 653 (A118), pp.23. ⟨10.1051/0004-6361/202141503⟩
We analyzed the surface of Vesta at visible wavelengths, using the data of the Visible and InfraRed mapping spectrometer (VIR) on board the Dawn spacecraft. We mapped the variations of various spectral parameters on the entire surface of the asteroid
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2d76f5517a626758b78942db1d8514aa
https://hal.archives-ouvertes.fr/hal-03354454
https://hal.archives-ouvertes.fr/hal-03354454
Akademický článek
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Autor:
Mauro Ciarniello, Andrea Raponi, S. De Angelis, Eleonora Ammannito, M. C. De Sanctis, M. Ferrari
Publikováno v:
Journal of Geophysical Research: Planets. 126