Poster Open Access

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

Nettelmann, Nadine


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{
  "description": "<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>", 
  "license": "https://creativecommons.org/licenses/by/4.0/legalcode", 
  "creator": [
    {
      "affiliation": "DLR-Berlin, PF-EPA", 
      "@type": "Person", 
      "name": "Nettelmann, Nadine"
    }
  ], 
  "url": "https://zenodo.org/record/5562545", 
  "datePublished": "2021-10-11", 
  "version": "1", 
  "@context": "https://schema.org/", 
  "identifier": "https://doi.org/10.5281/zenodo.5562545", 
  "@id": "https://doi.org/10.5281/zenodo.5562545", 
  "@type": "CreativeWork", 
  "name": "Structure and evolution of the tidally heated hot-Jupiter KELT-9b"
}
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