NASAのジュノー、木星の衛星イオの溶岩湖をクローズアップで見る(NASA’s Juno Gets a Close-Up Look at Lava Lakes on Jupiter’s Moon Io)

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2024-06-26 NASA

NASAのジュノー探査機の新しい発見により、木星の衛星イオに広がる溶岩湖と火山活動の詳細が明らかになりました。イオは1610年にガリレオ・ガリレイによって発見され、その後NASAのボイジャー1号が火山噴火を観測。ジュノーの赤外線オーロラマッパー(JIRAM)で取得されたデータにより、イオの表面がカルデラ状の溶岩湖で覆われていることが判明しました。2023年10月のフライバイでは、イオの表面の約3%が溶岩湖で覆われていることが示されました。赤外線画像により、湖の縁には溶岩の薄い輪が見られ、中央の溶岩が湖の壁にぶつかって崩れる様子が観察されました。この発見は、イオの火山活動と内部構造の理解を深めるものです。

<関連情報>

JUNO/JIRAMが観測したイオの熱い環 Hot rings on Io observed by Juno/JIRAM

Alessandro Mura,Federico Tosi,Francesca Zambon,Rosaly M. C. Lopes,Peter J. Mouginis-Mark,Heidi Becker,Gianrico Filacchione,Alessandra Migliorini,Candice. J. Hansen,Alberto Adriani,Francesca Altieri,Scott Bolton,Andrea Cicchetti,Elisa Di Mico,Davide Grassi,Raffaella Noschese,Alessandro Moirano,Madeline Pettine,Giuseppe Piccioni,Christina Plainaki,Julie Rathbun,Roberto Sordini &Giuseppe Sindoni
Communications Earth & Environment  Published:20 June 2024
DOI:https://doi.org/10.1038/s43247-024-01486-5

figure 2

 

Abstract

It has been thought that Io’s many paterae may contain lava lakes, but observations by NASA’s Galileo spacecraft at sufficiently high resolution were limited to a few locations, such as Loki Patera. Data acquired by NASA’s Juno mission in May 2023 reveal a common set of thermal characteristics for at least ten paterae on Io, with bright (hot) “thermal rings” around the perimeter of their floors. Loki, Surt, Fuchi, Amaterasu, Mulungu, Chors, and Dazhbog Patera, and four unnamed paterae, all show the same pattern of surface temperature. This new Juno/JIRAM data suggests that hot rings around paterae are a common phenomenon, and that they are indicative of active lava lakes. All the investigated paterae lack recent lava flows on their flanks, suggesting that at the time of observations, the level of the lake was not high enough to overflow the rim. These observations provide insight about the characteristics of paterae’s activity, which may involve either central upwelling of magma, or up-and-down “piston-like” vertical motion of the lake surface. Tidal forces, which are extreme at Io, could play a role as well. Future observations from Juno, particularly during the closest flybys, may indicate which mechanism is more plausible.

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