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DISCOVERY OF AN EXTENDED SODIUM ATMOSPHERE AROUND EUROPA

机译:围绕欧罗巴的扩展钠大气的发现

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摘要

EUROPA one of the satellites of Jupiter, has long been thought to be a dormant icy body(1), unlike its volcanically active neighbour, Io. Europa lies deep within Jupiter's magnetosphere, however, and is continuously bombarded by energetic ions, which modify the surface ices(2) and are probably responsible for creating Europa's tightly bound oxygen atmosphere(3,4). Here we report the discovery of an atmosphere of atomic sodium that extends to at least 25 times Europa's radius. We suggest that this sodium is originally released by Io's volcanoes, after which it is ionized in the magnetosphere and implanted into Europa's surface ice; subsequent sputtering of the ice by magnetospheric ions releases the sodium to form the extended atmosphere. Although sodium is a minor constituent of Europa's atmosphere, it traces the distribution of the major atmospheric components which are not themselves directly observable. The sodium and oxygen could represent the extremes of the distribution of the atmospheric components, with only the heaviest molecules (such as the oxygen) being tightly bound; alternatively the sodium might be in the form of an extended corona, analogous to Io's atmosphere. [References: 11]
机译:与木星活跃的邻国艾奥(Io)不同,欧洲木星(EUROPA)一直是木星的卫星之一,它一直处于休眠状态。然而,木卫二位于木星的磁层深处,并不断受到高能离子的轰击,这些离子改变了表面的冰(2),并可能造成了木卫二的紧密结合氧气氛(3,4)。在这里,我们报告发现了一种原子钠气氛,该气氛至少延伸到欧罗巴半径的25倍。我们建议这种钠最初是由艾奥火山释放的,然后在磁层中被离子化并植入欧罗巴的表层冰中。随后磁层离子对冰的溅射会释放钠,从而形成扩展的气氛。尽管钠是欧罗巴大气的次要成分,但它可以追踪主要大气成分的分布,而这些成分本身并不能直接观察到。钠和氧可能代表了大气成分的极端分布,只有最重的分子(例如氧)被紧密结合。另外,钠的形式可能类似于Io的大气,是扩展的电晕形式。 [参考:11]

著录项

  • 来源
    《Nature》 |1996年第6571期|p. 229-231|共3页
  • 作者

    Brown ME.; Hill RE.;

  • 作者单位

    CALTECH DIV GEOL & PLANETARY SCI MAIL STOP 170-25 PASADENA CA 91125 USA;

  • 收录信息 美国《科学引文索引》(SCI);美国《工程索引》(EI);美国《生物学医学文摘》(MEDLINE);美国《化学文摘》(CA);
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类 自然科学总论;
  • 关键词

    Plasma;

    机译:等离子体;

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