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These \u2018hot\u00a0Jupiter\u2019 planets are instead thought to have migrated inward from beyond the ice line and several viable migration channels have been proposed, including eccentricity excitation through angular-momentum exchange with a third body followed by tidally driven orbital circularization\n                    <jats:sup>2,3<\/jats:sup>\n                    . The discovery of the extremely eccentric (\n                    <jats:italic>e<\/jats:italic>\n                    \u2009=\u20090.93) giant exoplanet HD\u200980606\u2009b (ref.\u2009\n                    <jats:sup>4<\/jats:sup>\n                    ) provided observational evidence that hot Jupiters may have formed through this high-eccentricity tidal-migration pathway\n                    <jats:sup>5<\/jats:sup>\n                    . However, no similar hot-Jupiter progenitors have been found and simulations predict that one factor affecting the efficacy of this mechanism is exoplanet mass, as low-mass planets are more likely to be tidally disrupted during periastron passage\n                    <jats:sup>6\u20138<\/jats:sup>\n                    . Here we present spectroscopic and photometric observations of TIC\u2009241249530\u2009b, a high-mass, transiting warm Jupiter with an extreme orbital eccentricity of\n                    <jats:italic>e<\/jats:italic>\n                    \u2009=\u20090.94. The orbit of TIC\u2009241249530\u2009b is consistent with a history of eccentricity oscillations and a future tidal circularization trajectory. Our analysis of the mass and eccentricity distributions of the transiting-warm-Jupiter population further reveals a correlation between high mass and high eccentricity.\n                  <\/jats:p>","DOI":"10.1038\/s41586-024-07688-3","type":"journal-article","created":{"date-parts":[[2024,7,17]],"date-time":"2024-07-17T12:02:19Z","timestamp":1721217739000},"page":"50-54","update-policy":"https:\/\/doi.org\/10.1007\/springer_crossmark_policy","source":"Crossref","is-referenced-by-count":38,"title":["A hot-Jupiter progenitor on a super-eccentric retrograde orbit"],"prefix":"10.1038","volume":"632","author":[{"ORCID":"https:\/\/orcid.org\/0000-0002-5463-9980","authenticated-orcid":false,"given":"Arvind F.","family":"Gupta","sequence":"first","affiliation":[],"role":[{"vocabulary":"crossref","role":"author"}]},{"ORCID":"https:\/\/orcid.org\/0000-0003-3130-2282","authenticated-orcid":false,"given":"Sarah C.","family":"Millholland","sequence":"additional","affiliation":[],"role":[{"vocabulary":"crossref","role":"author"}]},{"ORCID":"https:\/\/orcid.org\/0009-0006-0871-1618","authenticated-orcid":false,"given":"Haedam","family":"Im","sequence":"additional","affiliation":[],"role":[{"vocabulary":"crossref","role":"author"}]},{"ORCID":"https:\/\/orcid.org\/0000-0002-3610-6953","authenticated-orcid":false,"given":"Jiayin","family":"Dong","sequence":"additional","affiliation":[],"role":[{"vocabulary":"crossref","role":"author"}]},{"ORCID":"https:\/\/orcid.org\/0000-0002-0323-4828","authenticated-orcid":false,"given":"Jonathan M.","family":"Jackson","sequence":"additional","affiliation":[],"role":[{"vocabulary":"crossref","role":"author"}]},{"ORCID":"https:\/\/orcid.org\/0000-0002-0810-3747","authenticated-orcid":false,"given":"Ilaria","family":"Carleo","sequence":"additional","affiliation":[],"role":[{"vocabulary":"crossref","role":"author"}]},{"given":"Jessica","family":"Libby-Roberts","sequence":"additional","affiliation":[],"role":[{"vocabulary":"crossref","role":"author"}]},{"given":"Megan","family":"Delamer","sequence":"additional","affiliation":[],"role":[{"vocabulary":"crossref","role":"author"}]},{"given":"Mark R.","family":"Giovinazzi","sequence":"additional","affiliation":[],"role":[{"vocabulary":"crossref","role":"author"}]},{"given":"Andrea S. 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