Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.

In Situ exploration of the giant planets

Autor: Don Banfield, Olivier Mousis, Mark Hofstadter, Leigh N. Fletcher, Sushil K. Atreya, Jean-Pierre Lebreton, Athena Coustenis, Francesca Ferri, Magali Deleuil, Peter Wurz, Kathleen Mandt, Thibault Cavalié, J. Hunter Waite, Thomas R. Spilker, Paul Hartogh, Heike Rauer, Kunio M. Sayanagi, Ethiraj Venkatapathy, Thierry Fouchet, Stas Barabash, Amy Simon, Tristan Guillot, R. Hueso, Jean-Baptiste Renard, Agustín Sánchez-Lavega, Michel Blanc, Richard M. Ambrosi, David H. Atkinson, Pascal Rannou, Georges Durry

Publikováno v: Experimental Astronomy
Experimental Astronomy, Springer Link, 2021, ⟨10.1007/s10686-021-09775-z⟩
Experimental Astronomy, springer Link, 2021, 39 p. ⟨10.1007/s10686-021-09775-z⟩
Experimental Astronomy, 2021, ⟨10.1007/s10686-021-09775-z⟩
Experimental Astronomy, 2021, 39 p. ⟨10.1007/s10686-021-09775-z⟩

Remote sensing observations suffer significant limitations when used to study the bulk atmospheric composition of the giant planets of our solar system. This impacts our knowledge of the formation of these planets and the physics of their atmospheres

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c12387c0d891da86289f939f36fe2895
https://hal.archives-ouvertes.fr/hal-03358205

Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.

The Nature and Composition of Jupiter's Building Blocks Derived from the Water Abundance Measurements by the Juno Spacecraft

Autor: Artyom Aguichine, Jonathan Lunine, Olivier Mousis

Publikováno v: apjl
apjl, 2021, 918 (2), pp.L23. ⟨10.3847/2041-8213/ac1d50⟩

The microwave radiometer aboard the Juno spacecraft provided a measurement of the water abundance found to range between 1 and 5.1 times the protosolar abundance of oxygen in the near-equatorial region of Jupiter. Here, we aim to combine this up-to-d

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::54d1d656eb80fab906cecc469f11bcb7
https://hal.science/hal-03585146

The water abundance in Jupiter’s equatorial zone

Autor: Michael Janssen, Paul G. Steffes, Fabiano Oyafuso, J. K. Arballo, Shannon Brown, Sidharth Misra, Jonathan I. Lunine, Amoree Hodges, Glenn S. Orton, Zhimeng Zhang, Liming Li, Sushil K. Atreya, Daniel Santos-Costa, Scott Bolton, Hunter Waite, Samuel Gulkis, Steven Levin, Cheng Li, Andrew P. Ingersoll, Tristan Guillot, Michael Allison, Virgil Adumitroaie, Amadeo Bellotti

Publikováno v: Nature Astronomy
Nature Astronomy, Nature Publishing Group, 2020, ⟨10.1038/s41550-020-1009-3⟩

Oxygen is the most common element after hydrogen and helium in Jupiter's atmosphere, and may have been the primary condensable (as water ice) in the protoplanetary disk. Prior to the Juno mission, in situ measurements of Jupiter's water abundance wer

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b3478fc29ad9445aac68fc50eb04a5e2
https://resolver.caltech.edu/CaltechAUTHORS:20191223-105236594