Zobrazeno 1 - 10
of 24
pro vyhledávání: '"Mikael Beuthe"'
Autor:
Antonio Genova, Sander Goossens, Edoardo Del Vecchio, Flavio Petricca, Mikael Beuthe, Mark Wieczorek, Gianluca Chiarolanza, Gaetano di Achille, Giuseppe Mitri, Ivan Di Stefano, Bernard Charlier, Erwan Mazarico, Peter James
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cd48725cb4f5b02cc2aea0a22caf40b9
https://hdl.handle.net/11573/1664612
https://hdl.handle.net/11573/1664612
Since being first visited by the spacecraft Cassini in 2005, the Saturnian moon Enceladus has attracted far more attention than could be guessed from its modest size and lack of atmosphere, compared to its giant neighbour Titan. The reason for this s
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::47a7772cbc786d5e66107523fa9362d4
https://doi.org/10.5194/epsc2022-1042
https://doi.org/10.5194/epsc2022-1042
Autor:
Mikael Beuthe
Publikováno v:
Geophysical Journal International. 227:693-716
In modern geodynamics, isostasy can be viewed either as the static equilibrium of the crust that minimizes deviatoric stresses, or as a dynamic process resulting from the viscous relaxation of the non-hydrostatic crustal shape. Paper I gave a general
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6e3cd296e3a53c0a5bff98c2071d1c9d
https://doi.org/10.1093/gji/ggab241
https://doi.org/10.1093/gji/ggab241
Autor:
Sebastien Le Maistre, Veronique Dehant, Rose-Marie Baland, Mikael Beuthe, Alfonso Caldiero, Valerio Filice, Marta Goli, Marie-Julie Péters, Bertrand Steenput, Attilio Rivoldini, Ertan Ümit, Tim Van Hoolst, Marie Yseboodt
Publikováno v:
Proc. EPSC 2022 Meeting
LaRa is a radio-science instrument that is ready to fly and was part of the science payload of the surface platform of the ExoMars mission. Now that ExoMars is suspended, LaRa will need to find another mission to go to the Martian system (or elsewher
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5bca58287db042979dc8ddf43c9671f6
Autor:
Mikael Beuthe
Publikováno v:
Icarus. 332:66-91
Tidal heating is the prime suspect behind Enceladus's south polar heating anomaly and global subsurface ocean. No model of internal tidal dissipation, however, can explain at the same time the total heat budget and the focusing of the energy at the s
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cf746e75bf4e78c7aab5dfc591944107
https://doi.org/10.1016/j.icarus.2019.05.035
https://doi.org/10.1016/j.icarus.2019.05.035
Autor:
Mikael Beuthe
Dissipation of ocean potential energy is proposed by Tyler (2020) as a new mechanism leading to possible high-power states for Enceladus. I show here that this process actually results from viscoelastic dissipation within the crust. For plausible val
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3262862e80da46f34ff633148f764f81
http://arxiv.org/abs/2011.14800
http://arxiv.org/abs/2011.14800
Autor:
Mikael Beuthe
Isostasy explains why observed gravity anomalies are generally much weaker than what is expected from topography alone, and why planetary crusts can support high topography without breaking up. Classical isostasy, however, neglects internal stresses
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::17b11f95595d217a805e0a53f1e50a05
Publikováno v:
Geophysical Research Letters
Mercury's crust has a complex structure resulting from a billion years of volcanism. The surface variations in chemical composition have been identified from orbit by the spacecraft MESSENGER. Combining these measurements with laboratory experiments
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1d753f5d74ffa03cd1789dfea4aac4a6
Autor:
Mikael Beuthe
Publikováno v:
Icarus. 302:145-174
The geologic activity at Enceladus's south pole remains unexplained, though tidal deformations are probably the ultimate cause. Recent gravity and libration data indicate that Enceladus's icy crust floats on a global ocean, is rather thin, and has a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::166b78f6c897b57b35b29880aa0e357a
https://doi.org/10.1016/j.icarus.2017.11.009
https://doi.org/10.1016/j.icarus.2017.11.009
Publikováno v:
Journal of Geophysical Research. Planets
Journal of Geophysical Research. Planets, Wiley-Blackwell, 2019, 124 (5), pp.1410-1432. ⟨10.1029/2018JE005909⟩
Journal of Geophysical Research: Planets
Journal of Geophysical Research. Planets, Wiley-Blackwell, 2019, 124 (5), pp.1410-1432. ⟨10.1029/2018JE005909⟩
Journal of Geophysical Research: Planets
International audience; Below the lithospheres of the terrestrial planets, dwarf planets, and moons, density interfaces adjust over geologic time to align with surfaces of constant gravitational potential. It is well known that the shape of such hydr
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c6166371775f345532ec6e11c76cc5b4
https://doi.org/10.1029/2018je005909
https://doi.org/10.1029/2018je005909