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木卫二表面存在内源性一氧化碳冰混合物且未检测到羽流活动。

Endogenous CO ice mixture on the surface of Europa and no detection of plume activity.

作者信息

Villanueva G L, Hammel H B, Milam S N, Faggi S, Kofman V, Roth L, Hand K P, Paganini L, Stansberry J, Spencer J, Protopapa S, Strazzulla G, Cruz-Mermy G, Glein C R, Cartwright R, Liuzzi G

机构信息

NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA.

Association of Universities for Research in Astronomy, Washington, DC 20004, USA.

出版信息

Science. 2023 Sep 22;381(6664):1305-1308. doi: 10.1126/science.adg4270. Epub 2023 Sep 21.

Abstract

Jupiter's moon Europa has a subsurface ocean beneath an icy crust. Conditions within the ocean are unknown, and it is unclear whether it is connected to the surface. We observed Europa with the James Webb Space Telescope (JWST) to search for active release of material by probing its surface and atmosphere. A search for plumes yielded no detection of water, carbon monoxide, methanol, ethane, or methane fluorescence emissions. Four spectral features of carbon dioxide (CO) ice were detected; their spectral shapes and distribution across Europa's surface indicate that the CO is mixed with other compounds and concentrated in Tara Regio. The CO absorption is consistent with an isotopic ratio of C/C = 83 ± 19. We interpret these observations as indicating that carbon is sourced from within Europa.

摘要

木星的卫星木卫二在其冰壳之下有一个地下海洋。海洋内部的情况未知,并且尚不清楚它是否与表面相连。我们使用詹姆斯·韦布空间望远镜(JWST)对木卫二进行观测,通过探测其表面和大气层来寻找物质的活跃释放。对羽流的搜索未检测到水、一氧化碳、甲醇、乙烷或甲烷的荧光发射。检测到了二氧化碳(CO)冰的四个光谱特征;它们的光谱形状和在木卫二表面的分布表明,CO与其他化合物混合并集中在塔拉地区。CO的吸收与C/C = 83 ± 19的同位素比率一致。我们将这些观测结果解释为表明碳源自木卫二内部。

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