October 11, 2021 Poster Open Access

Nettelmann, Nadine

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  <identifier identifierType="DOI">10.5281/zenodo.5562545</identifier>
  <creators>
    <creator>
      <creatorName>Nettelmann, Nadine</creatorName>
      <givenName>Nadine</givenName>
      <familyName>Nettelmann</familyName>
      <affiliation>DLR-Berlin, PF-EPA</affiliation>
    </creator>
  </creators>
  <titles>
    <title>Structure and evolution of the tidally heated hot-Jupiter KELT-9b</title>
  </titles>
  <publisher>Zenodo</publisher>
  <publicationYear>2021</publicationYear>
  <dates>
    <date dateType="Issued">2021-10-11</date>
  </dates>
  <resourceType resourceTypeGeneral="Text">Poster</resourceType>
  <alternateIdentifiers>
    <alternateIdentifier alternateIdentifierType="url">https://zenodo.org/record/5562545</alternateIdentifier>
  </alternateIdentifiers>
  <relatedIdentifiers>
    <relatedIdentifier relatedIdentifierType="DOI" relationType="IsVersionOf">10.5281/zenodo.5562544</relatedIdentifier>
    <relatedIdentifier relatedIdentifierType="URL" relationType="IsPartOf">https://zenodo.org/communities/plato2021</relatedIdentifier>
  </relatedIdentifiers>
  <version>1</version>
  <rightsList>
    <rights rightsURI="https://creativecommons.org/licenses/by/4.0/legalcode">Creative Commons Attribution 4.0 International</rights>
    <rights rightsURI="info:eu-repo/semantics/openAccess">Open Access</rights>
  </rightsList>
  <descriptions>
    <description descriptionType="Abstract">&lt;p&gt;The hot Jupiter KELT-9b is observed to have a strong intrinsic heat flux T_int ~ 2400 +/- 800 K. However, requesting a bulk metallicity&amp;nbsp; Z&amp;lt;20% requires significantly lower T_int. To resolve this discrepancy, we suggest (obliquity) tidal heating in a shell and a static k2 &amp;lt; 0.1.&lt;/p&gt;

&lt;p&gt;&amp;nbsp;&lt;/p&gt;</description>
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