Zobrazeno 1 - 10
of 448
pro vyhledávání: '"Ice giant"'
Autor:
Daniel J. Gershman, Gina A. DiBraccio
Publikováno v:
Geophysical Research Letters, Vol 51, Iss 15, Pp n/a-n/a (2024)
Abstract The long‐standing “energy crisis” at the giant planets refers to the anomalous heating of planetary thermospheres compared to the available energy from solar irradiance. The coupling between planetary magnetospheres and their upper atm
Externí odkaz:
https://doaj.org/article/e15d8c3dfb664226a01cebe99e1d2978
Autor:
Xin Cao, Xiangning Chu, Hsiang-Wen Hsu, Hao Cao, Weijie Sun, Lucas Liuzzo, Jasper Halekas, Carol Paty, Feng Chu, Omakshi Agiwal, Lauren Blum, Frank Crary, Ian J. Cohen, Peter Delamere, Mark Hofstadter, George Hospodarsky, Cooper John, Peter Kollmann, Elena Kronberg, William Kurth, Laurent Lamy, Dong Lin, Wen Li, Xuanye Ma, David Malaspina, Michiko Morooka, Tom Nordheim, Frank Postberg, Andrew Poppe, Cartwright Richard, Suranga Ruhunusiri, Krista Soderlund, James O'Donoghue, Ferdinand Plaschke
Publikováno v:
Frontiers in Astronomy and Space Sciences, Vol 11 (2024)
The magnetospheric systems of ice giants, as the ideal and the unique template of a typical class of exoplanets, have not been sufficiently studied in the past decade. The complexity of these asymmetric and extremely dynamic magnetospheres provides u
Externí odkaz:
https://doaj.org/article/8463fd388762420fa033023837f113ca
Akademický článek
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Akademický článek
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So far no designated mission to either of the two ice giants, Uranus and Neptune, exists. Almost all of our gathered information on these planets comes from remote sensing. In recent years, NASA and ESA have started planning for future mission to Ura
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::86280f022fc208c2b48c74983d04abf7
http://arxiv.org/abs/2306.09645
http://arxiv.org/abs/2306.09645
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⟩
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
https://doi.org/10.1007/s10686-021-09759-z
Autor:
Williams, Ashleigh
Publikováno v:
School Library Journal. Dec2021, Vol. 67 Issue 12, p84-84. 1/6p.
Autor:
Philip Horzempa
The key to the exploration of the Ice Giant planets is avoiding cutting edge technology. Complexity produces delay and financial roadblocks. Simple robot scouts can be launched in time to utilize gravity assists from Jupiter in the early 2030s. Deman
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b2b8793db33e22dd46a90ae48642172b
http://arxiv.org/abs/2212.00803
http://arxiv.org/abs/2212.00803
Publikováno v:
Nature Physics
In the phase diagram of water, superionic ices with highly mobile protons within the stable oxygen sublattice have been predicted at high pressures. However, the existence of superionic ices and the location of the melting line have been challenging
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fbcd4027a37356a0045b3f5cce9a9b50
https://doi.org/10.1038/s41567-021-01351-8
https://doi.org/10.1038/s41567-021-01351-8
Publikováno v:
Journal of Spacecraft and Rockets. 58:1477-1486
Reentry radiation is one of the key phenomena to take into account while designing an Entry Descent and Landing (EDL) phase for sample return and some gas/ice giants’ missions. In the case of an ablative thermal protective system (TPS), the physico
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6d1bb3c543a7afc3a8051464cb88635d
https://doi.org/10.2514/1.a34969
https://doi.org/10.2514/1.a34969