Southwest Research Institute, San Antonio, TX, USA.
Science. 2014 Jan 10;343(6167):171-4. doi: 10.1126/science.1247051. Epub 2013 Dec 12.
In November and December 2012, the Hubble Space Telescope (HST) imaged Europa's ultraviolet emissions in the search for vapor plume activity. We report statistically significant coincident surpluses of hydrogen Lyman-α and oxygen OI 130.4-nanometer emissions above the southern hemisphere in December 2012. These emissions were persistently found in the same area over the 7 hours of the observation, suggesting atmospheric inhomogeneity; they are consistent with two 200-km-high plumes of water vapor with line-of-sight column densities of about 10(20) per square meter. Nondetection in November 2012 and in previous HST images from 1999 suggests varying plume activity that might depend on changing surface stresses based on Europa's orbital phases. The plume was present when Europa was near apocenter and was not detected close to its pericenter, in agreement with tidal modeling predictions.
2012 年 11 月和 12 月,哈勃太空望远镜(HST)对木卫二的紫外发射进行成像,以寻找水汽羽流活动。我们报告了在 2012 年 12 月南半球氢莱曼阿尔法和氧 OI 130.4 纳米发射同时出现显著的过剩现象。这些排放物在观测的 7 小时内持续出现在同一区域,表明大气不均匀;它们与两个 200 公里高的水蒸气羽流一致,视线上的柱密度约为每平方米 10(20)。2012 年 11 月和 1999 年之前的 HST 图像没有探测到,表明羽流活动可能随木卫二的轨道相位而变化,这可能取决于表面应力的变化。当木卫二接近远地点时羽流存在,而在接近其近日点时未检测到,这与潮汐模型的预测一致。