Journal article Open Access

A post-Galileo view of Io's interior

Keszthelyi, Laszlo; Jaeger, Windy L.; Turtle, Elizabeth P.; Milazzo, Moses; Radebaugh, Jani


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  <identifier identifierType="URL">https://zenodo.org/record/1259017</identifier>
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    <creator>
      <creatorName>Keszthelyi, Laszlo</creatorName>
      <givenName>Laszlo</givenName>
      <familyName>Keszthelyi</familyName>
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    <creator>
      <creatorName>Jaeger, Windy L.</creatorName>
      <givenName>Windy L.</givenName>
      <familyName>Jaeger</familyName>
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    <creator>
      <creatorName>Turtle, Elizabeth P.</creatorName>
      <givenName>Elizabeth P.</givenName>
      <familyName>Turtle</familyName>
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    <creator>
      <creatorName>Milazzo, Moses</creatorName>
      <givenName>Moses</givenName>
      <familyName>Milazzo</familyName>
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    <creator>
      <creatorName>Radebaugh, Jani</creatorName>
      <givenName>Jani</givenName>
      <familyName>Radebaugh</familyName>
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  <titles>
    <title>A post-Galileo view of Io's interior</title>
  </titles>
  <publisher>Zenodo</publisher>
  <publicationYear>2004</publicationYear>
  <dates>
    <date dateType="Issued">2004-05-01</date>
  </dates>
  <resourceType resourceTypeGeneral="JournalArticle"/>
  <alternateIdentifiers>
    <alternateIdentifier alternateIdentifierType="url">https://zenodo.org/record/1259017</alternateIdentifier>
  </alternateIdentifiers>
  <relatedIdentifiers>
    <relatedIdentifier relatedIdentifierType="DOI" relationType="IsIdenticalTo">10.1016/j.icarus.2004.01.005</relatedIdentifier>
  </relatedIdentifiers>
  <rightsList>
    <rights rightsURI="https://creativecommons.org/publicdomain/zero/1.0/legalcode">Creative Commons Zero v1.0 Universal</rights>
    <rights rightsURI="info:eu-repo/semantics/openAccess">Open Access</rights>
  </rightsList>
  <descriptions>
    <description descriptionType="Abstract">We present a self-consistent model for the interior of Io, taking the recent Galileo data into account. In this model, Io has a completely molten core, substantially molten mantle, and a very cold lithosphere. Heat from magmatic activity can mobilize volatile compounds such as SO2 in the lithosphere, and the movement of such cryogenic fluids may be important in the formation of surface features including sapping scarps and paterae.</description>
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