October 11, 2021 Poster Open Access

Nettelmann, Nadine

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  <dc:creator>Nettelmann, Nadine</dc:creator>
  <dc:date>2021-10-11</dc:date>
  <dc:description>The hot Jupiter KELT-9b is observed to have a strong intrinsic heat flux T_int ~ 2400 +/- 800 K. However, requesting a bulk metallicity  Z&lt;20% requires significantly lower T_int. To resolve this discrepancy, we suggest (obliquity) tidal heating in a shell and a static k2 &lt; 0.1.

 </dc:description>
  <dc:identifier>https://zenodo.org/record/5562545</dc:identifier>
  <dc:identifier>10.5281/zenodo.5562545</dc:identifier>
  <dc:identifier>oai:zenodo.org:5562545</dc:identifier>
  <dc:relation>doi:10.5281/zenodo.5562544</dc:relation>
  <dc:relation>url:https://zenodo.org/communities/plato2021</dc:relation>
  <dc:rights>info:eu-repo/semantics/openAccess</dc:rights>
  <dc:rights>https://creativecommons.org/licenses/by/4.0/legalcode</dc:rights>
  <dc:title>Structure and evolution of the tidally heated hot-Jupiter KELT-9b</dc:title>
  <dc:type>info:eu-repo/semantics/conferencePoster</dc:type>
  <dc:type>poster</dc:type>
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