A subsolar oxygen abundance or a radiative region deep in Jupiter revealed by thermochemical modelling

Autor: T. Cavalié, J. Lunine, O. Mousis

Jupiter's deep abundances help to constrain the formation history of the planet and the environment of the protoplanetary nebula. Juno recently measured Jupiter's deep oxygen abundance near the equator to be 2.2$_{-2.1}^{+3.9}$ times the protosolar v

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::71c96b79fb8cf8492f1a5d3eeb0e0426
http://arxiv.org/abs/2305.13949

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Moonraker -- Enceladus Multiple Flyby Mission

Autor: O. Mousis, A. Bouquet, Y. Langevin, N. André, H. Boithias, G. Durry, F. Faye, P. Hartogh, J. Helbert, L. Iess, S. Kempf, A. Masters, F. Postberg, J.-B. Renard, P. Vernazza, A. Vorburger, P. Wurz, D. H. Atkinson, S. Barabash, M. Berthomier, J. Brucato, M. Cable, J. Carter, S. Cazaux, A. Coustenis, G. Danger, V. Dehant, T. Fornaro, P. Garnier, T. Gautier, O. Groussin, L. Z. Hadid, J.-C. Ize, I. Kolmasova, J.-P. Lebreton, S. Le Maistre, E. Lellouch, J. I. Lunine, K. E. Mandt, Z. Martins, D. Mimoun, Q. Nenon, G. M. Muñoz Caro, P. Rannou, H. Rauer, P. Schmitt-Kopplin, A. Schneeberger, M. Simons, K. Stephan, T. Van Hoolst, J. Vaverka, M. Wieser, L. Wörner

Publikováno v: Mousis, O.; Bouquet, A.; Langevin, Y.; André, N.; Boithias, H.; Durry, G.; Faye, F.; Hartogh, P.; Helbert, J.; Iess, L.; Kempf, S.; Masters, A.; Postberg, F.; Renard, J.-B.; Vernazza, P.; Vorburger, A.; Wurz, P.; Atkinson, D. H.; Barabash, S.; Berthomier, M.; ... (2022). Moonraker: Enceladus Multiple Flyby Mission. The planetary science journal, 3(12), p. 268. IOP Publishing 10.3847/PSJ/ac9c03
The Planetary Science Journal, Vol. 3, no.12, p. 268 (2022)
The Planetary Science Journal, 3(12):268
The Planetary Science Journal
The Planetary Science Journal, 2022, 3, 268 (12pp). ⟨10.3847/psj/ac9c03⟩

Enceladus, an icy moon of Saturn, possesses an internal water ocean and jets expelling ocean material into space. Cassini investigations indicated that the subsurface ocean could be a habitable environment having a complex interaction with the rocky

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::098b4c93a9acdc706ca949f270e335bc
http://arxiv.org/abs/2211.00721

Ice giant system exploration within ESA’s Voyage 2050

Autor: Nadine Nettleman, Paolo Tortora, Jonathan J. Fortney, Ricardo Hueso, David Andrews, Jürgen Schmidt, Francesca Ferri, Adam Masters, Ravit Helled, Gabriel Tobie, O. Mousis, Nicolas André, Léa Griton, Michele T. Bannister, Diego Turrini, Amy Simon, Yohai Kaspi, Paul Hartogh, Geraint H. Jones, Thibault Cavalié, Laurent Lamy, Elias Roussos, Christina Plainaki, Leigh N. Fletcher, Julianne I. Moses, Emma J. Bunce, Davide Grassi, Sébastien Charnoz, Federico Tosi, Henrik Melin

Publikováno v: Experimental Astronomy
Experimental Astronomy, Springer Link, 2021, ⟨10.1007/s10686-021-09759-z⟩

Of all the myriad environments in our Solar System, the least explored are the distant Ice Giants Uranus and Neptune, and their diverse satellite and ring systems. These ‘intermediate-sized’ worlds are the last remaining class of Solar System pla

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7165224822bb6e78555aa262088c61ea
https://doi.org/10.1007/s10686-021-09759-z

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