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>", 
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