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The inferred subsurface oceans of the icy moons of Jupiter and Saturn, in particular Europa and Enceladus, may contain conditions suitable for life. Plumes of material have been detected from Enceladus and may also be present on Europa. These plumes
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::addb8ed6c296f851b93c1e8b54f5bd34
https://doi.org/10.5194/epsc2021-518
https://doi.org/10.5194/epsc2021-518
Introduction: The potential habitability of the icy moons of Jupiter and Saturn, in particular Europa and Enceladus, has been hotly debated in recent years. There is evidence of subsurface liquid water oceans [1], and complex organic molecules (>200
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d6160c8ef262385102cb1ce42dd0b5f4
https://doi.org/10.5194/epsc2020-143
https://doi.org/10.5194/epsc2020-143
Publikováno v:
Icarus. 206:755-763
A hexagonal structure has been observed at ∼76°N on Saturn since the 1980s (Godfrey, D.A. [1988]. Icarus 76, 335-356). Recent images by Cassini (Baines, K., Momary, T., Roos-Serote, M., Atreya, S., Brown, R., Buratti, B., Clark, R., Nicholson, P.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2968b7fe217cea3b65613e213ca1ff33
https://doi.org/10.1016/j.icarus.2009.10.022
https://doi.org/10.1016/j.icarus.2009.10.022
