Poster Open Access

Structure and evolution of the tidally heated hot-Jupiter KELT-9b

Nettelmann, Nadine


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{
  "publisher": "Zenodo", 
  "DOI": "10.5281/zenodo.5562545", 
  "title": "Structure and evolution of the tidally heated hot-Jupiter KELT-9b", 
  "issued": {
    "date-parts": [
      [
        2021, 
        10, 
        11
      ]
    ]
  }, 
  "abstract": "<p>The hot Jupiter KELT-9b is observed to have a strong intrinsic heat flux T_int ~ 2400 +/- 800 K. However, requesting a bulk metallicity&nbsp; 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.</p>\n\n<p>&nbsp;</p>", 
  "author": [
    {
      "family": "Nettelmann, Nadine"
    }
  ], 
  "version": "1", 
  "type": "graphic", 
  "id": "5562545"
}
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