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Monitoring Volcanic Activity on Io

Monitoring Volcanic Activity on Io
监测木卫一上的火山活动
批准号:
0406275
负责人:
Imke de Pater
金额:
$0.0万
依托单位国家:
美国
项目类别:
Continuing Grant
财政年份:
2004
资助国家:
美国
项目状态:
已结题
起止时间:
2004-06-01 至 2009-10-31

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中文摘要
翻译
帕特里奥是太阳系中最引人注目的天体之一,它有潮汐加热驱动的火山以及与木星磁层的复杂相互作用。尽管航天器对这颗卫星进行了广泛的研究,但仍有许多问题没有得到解答。特别是加热和热损失过程没有得到详细的了解。为什么某些火山与气体羽流有关,而其他火山则完全没有,这也是一个谜。如果了解了火山的频率、空间分布和喷发方式,这些问题可能最终得到解答。这些参数只能通过在大型地面望远镜上使用自适应光学(AO)技术从地面监测Io来获得。Dr. De Pater和她的合作者将继续在夏威夷莫纳克亚山的凯克望远镜,夏威夷和智利的双子座望远镜,智利的甚大望远镜,利克天文台的3米望远镜,以及夏威夷莫纳克亚山的红外望远镜设施(IRTF)进行高分辨率观测项目。这可能是绘制木卫一上正在进行的火山活动和图表变化的唯一方法。只有通过极好的时间覆盖,才能对总热流的数量和变化以及这种活动的纬度和纵向分布设定限制。这些限制将与通过火山热模型和潮汐加热模型得出的喷发率进行比较。学生和公众都喜欢木卫一,因为它有巨大的火山。它是一个理想的公开演讲和课堂教学的主题,化学,物理,地球物理学和天文学可以结合在一起。研究生和本科生将参与这个项目的数据处理和分析技术。夏威夷学生将参与IRTF的Io观测。***
英文摘要
AST 0406275De PaterIo, with its tidal-heating driven volcanoes and complex interaction with Jupiter's magnetosphere, is one of the most remarkable bodies in the solar system. Although the satellite has been studied extensively by spacecraft, many questions remain unanswered. In particular the heating and heat loss processes are not understood in any detail. It also is still a mystery why certain volcanoes are associated with gas plumes and others are not at all. These questions might be answered ultimately if the frequency, spatial distribution, and eruption style of volcanoes are known. These parameters can only be derived by monitoring Io from the ground using Adaptive Optics (AO) techniques on large ground-based telescopes. Dr. De Pater and her collaborators will continue a program of high resolution observations with the Keck telescopes, on Mauna Kea, Hawaii, and an extension to the Gemini telescopes, in Hawaii and Chile, the Very Large Telescope, in Chile, the 3-meter telescope at Lick Observatory, and the Infrared Telescope Facility (IRTF), on Mauna Kea, Hawaii. This may be the only way to map ongoing volcanic activity and chart changes on Io. Only through excellent temporal coverage can one set limits on the amount of, and variations in, the total heat flow and the latitudinal and longitudinal distribution of this activity. These limits will be compared with those derived from eruption rates via volcano thermal models and with tidal heating models. Students and the public love Io with its giant volcanoes. It is an ideal subject for public presentations and for classroom teaching, where chemistry, physics, geophysics, and astronomy can be combined. Graduate and undergraduate students will be involved in the data processing and analysis techniques on this project. Hawaiian students will be involved in Io observations at the IRTF. ***
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Collaborative Research: Characterizing the Galilean satellite (sub)surfaces from radio observations
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    2308281
  • 项目类别:
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  • 资助金额:
    $10.65万
  • 财政年份:
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  • 依托单位:
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    1615004
  • 项目类别:
    Standard Grant
  • 资助金额:
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  • 财政年份:
    2016
  • 负责人:
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  • 依托单位:
A Multi-Wavelength Observing Program of Io Using Adaptive Optics and Interferometric Techniques
  • 批准号:
    1313485
  • 项目类别:
    Continuing Grant
  • 资助金额:
    $45.55万
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    2013
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Titan: High Angular Resolution Synergistic Groundbased Observations during the Cassini Era
  • 批准号:
    1008788
  • 项目类别:
    Standard Grant
  • 资助金额:
    $45.85万
  • 财政年份:
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  • 负责人:
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  • 依托单位:
海外基金