{"id":109530,"date":"2020-07-05T05:22:52","date_gmt":"2020-07-05T12:22:52","guid":{"rendered":"https:\/\/lifeboat.com\/blog\/2020\/07\/a-remnant-planetary-core-in-the-hot-neptune-desert"},"modified":"2020-07-05T05:22:52","modified_gmt":"2020-07-05T12:22:52","slug":"a-remnant-planetary-core-in-the-hot-neptune-desert","status":"publish","type":"post","link":"https:\/\/lifeboat.com\/blog\/2020\/07\/a-remnant-planetary-core-in-the-hot-neptune-desert","title":{"rendered":"A remnant planetary core in the hot-Neptune desert"},"content":{"rendered":"<p><a class=\"aligncenter blog-photo\" href=\"https:\/\/lifeboat.com\/blog.images\/a-remnant-planetary-core-in-the-hot-neptune-desert.jpg\"><\/a><\/p>\n<p>The interiors of giant planets remain poorly understood. Even for the planets in the Solar System, difficulties in observation lead to large uncertainties in the properties of planetary cores. Exoplanets that have undergone rare evolutionary processes provide a route to understanding planetary interiors. Planets found in and near the typically barren hot-Neptune \u2018desert\u2019<sup><a data-track=\"click\" data-track-action=\"reference anchor\" data-track-label=\"link\" data-test=\"citation-ref\" aria-label=\"Reference 1\" title=\"Szab\u00f3, G. M. & Kiss, L. L. A short-period censor of sub-Jupiter mass exoplanets with low density. Astrophys. J. Lett. 727, L44 (2011).\" href=\"https:\/\/www.nature.com\/articles\/s41586-020-2421-7#ref-CR1\" id=\"ref-link-section-d39216e2310\">1<\/a>,<a data-track=\"click\" data-track-action=\"reference anchor\" data-track-label=\"link\" data-test=\"citation-ref\" aria-label=\"Reference 2\" title=\"Owen, J. E. & Lai, D. Photoevaporation and high-eccentricity migration created the sub-Jovian desert. Mon. Not. R. Astron. Soc. 479, 5012&ndash;5021 (2018).\" href=\"https:\/\/www.nature.com\/articles\/s41586-020-2421-7#ref-CR2\" id=\"ref-link-section-d39216e2313\">2<\/a><\/sup> (a region in mass\u2013radius space that contains few planets) have proved to be particularly valuable in this regard. These planets include HD149026b<sup><a data-track=\"click\" data-track-action=\"reference anchor\" data-track-label=\"link\" data-test=\"citation-ref\" aria-label=\"Reference 3\" title=\"Sato, B. et al. The N2K Consortium. II. A transiting hot Saturn around HD 149026 with a large dense core. Astrophys. J. 633, 465&ndash;473 (2005).\" href=\"https:\/\/www.nature.com\/articles\/s41586-020-2421-7#ref-CR3\" id=\"ref-link-section-d39216e2317\">3<\/a><\/sup>, which is thought to have an unusually massive core, and recent discoveries such as LTT9779b<sup><a data-track=\"click\" data-track-action=\"reference anchor\" data-track-label=\"link\" data-test=\"citation-ref\" aria-label=\"Reference 4\" title=\"Jenkins, J. TESS Discovery of the first ultra hot Neptune, LTT9779b. In AAS\/Division for Extreme Solar Systems Abstracts Vol. 51, 103.07 (American Astronomical Society, 2019).\" href=\"https:\/\/www.nature.com\/articles\/s41586-020-2421-7#ref-CR4\" id=\"ref-link-section-d39216e2321\">4<\/a><\/sup> and NGTS-4b<sup><a data-track=\"click\" data-track-action=\"reference anchor\" data-track-label=\"link\" data-test=\"citation-ref\" aria-label=\"Reference 5\" title=\"West, R. G. et al. NGTS-4b: a sub-Neptune transiting in the desert. Mon. Not. R. Astron. Soc. 486, 5094&ndash;5103 (2019).\" href=\"https:\/\/www.nature.com\/articles\/s41586-020-2421-7#ref-CR5\" id=\"ref-link-section-d39216e2325\">5<\/a><\/sup>, on which photoevaporation has removed a substantial part of their outer atmospheres. Here we report observations of the planet TOI-849b, which has a radius smaller than Neptune\u2019s but an anomalously large mass of \\(39.1{\\,}_{-2.6}^{+2.7}\\) Earth masses and a density of \\(5.2{\\,}_{-0.8}^{+0.7}\\) grams per cubic centimetre, similar to Earth\u2019s. Interior-structure models suggest that any gaseous envelope of pure hydrogen and helium consists of no more than \\({3.9}_{-0.9}^{+0.8}\\) per cent of the total planetary mass. The planet could have been a gas giant before undergoing extreme mass loss via thermal self-disruption or giant planet collisions, or it could have avoided substantial gas accretion, perhaps through gap opening or late formation<sup><a data-track=\"click\" data-track-action=\"reference anchor\" data-track-label=\"link\" data-test=\"citation-ref\" aria-label=\"Reference 6\" title=\"Lee, E. J. The boundary between gas-rich and gas-poor planets. Astrophys. J. 878, 36 (2019).\" href=\"https:\/\/www.nature.com\/articles\/s41586-020-2421-7#ref-CR6\" id=\"ref-link-section-d39216e2383\">6<\/a><\/sup>. Although photoevaporation rates cannot account for the mass loss required to reduce a Jupiter-like gas giant, they can remove a small (a few Earth masses) hydrogen and helium envelope on timescales of several billion years, implying that any remaining atmosphere on TOI-849b is likely to be enriched by water or other volatiles from the planetary interior. We conclude that TOI-849b is the remnant core of a giant planet.<\/p>\n","protected":false},"excerpt":{"rendered":"<p>The interiors of giant planets remain poorly understood. Even for the planets in the Solar System, difficulties in observation lead to large uncertainties in the properties of planetary cores. Exoplanets that have undergone rare evolutionary processes provide a route to understanding planetary interiors. Planets found in and near the typically barren hot-Neptune \u2018desert\u20191,2 (a region [\u2026]<\/p>\n","protected":false},"author":427,"featured_media":0,"comment_status":"open","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[8],"tags":[],"class_list":["post-109530","post","type-post","status-publish","format-standard","hentry","category-space"],"_links":{"self":[{"href":"https:\/\/lifeboat.com\/blog\/wp-json\/wp\/v2\/posts\/109530","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/lifeboat.com\/blog\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/lifeboat.com\/blog\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/lifeboat.com\/blog\/wp-json\/wp\/v2\/users\/427"}],"replies":[{"embeddable":true,"href":"https:\/\/lifeboat.com\/blog\/wp-json\/wp\/v2\/comments?post=109530"}],"version-history":[{"count":0,"href":"https:\/\/lifeboat.com\/blog\/wp-json\/wp\/v2\/posts\/109530\/revisions"}],"wp:attachment":[{"href":"https:\/\/lifeboat.com\/blog\/wp-json\/wp\/v2\/media?parent=109530"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/lifeboat.com\/blog\/wp-json\/wp\/v2\/categories?post=109530"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/lifeboat.com\/blog\/wp-json\/wp\/v2\/tags?post=109530"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}