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Several planet candidates have recently been identified orbiting white dwarfs\n                    <jats:sup>1\u20134<\/jats:sup>\n                    , demonstrating that planets can survive the stellar post-main-sequence stage intact. Little is known about the atmospheric composition of post-main-sequence planets, with the most evolved transiting planets with atmospheric detections so far orbiting subgiants\n                    <jats:sup>5,6<\/jats:sup>\n                    . Here we report an atmospheric detection for the white dwarf planet WD\u20091856\u2009b, achieved through transmission spectroscopy with the James Webb Space Telescope (JWST) Near-Infrared Spectrograph (NIRSpec) PRISM. Our 0.5\u20135.0-\u03bcm spectrum reveals the presence of hydrocarbons (odds ratio of 167:1\u20135,377:1, with CH\n                    <jats:sub>4<\/jats:sub>\n                    preferred at 17:1\u201330:1), aerosols (2\u2009\u00d7\u200910\n                    <jats:sup>5<\/jats:sup>\n                    :1\u20132\u2009\u00d7\u200910\n                    <jats:sup>6<\/jats:sup>\n                    :1) and thermal emission from the planetary nightside (2\u2009\u00d7\u200910\n                    <jats:sup>63<\/jats:sup>\n                    :1\u20132\u2009\u00d7\u200910\n                    <jats:sup>73<\/jats:sup>\n                    :1). Our spectral analysis constrains the mass of WD\u20091856\u2009b to 4.3\u201310.9\u2009\n                    <jats:italic>M<\/jats:italic>\n                    <jats:sub>J<\/jats:sub>\n                    , finds a carbon-enriched atmosphere (with a CH\n                    <jats:sub>4<\/jats:sub>\n                    abundance of approximately 7%) and an effective temperature exceeding the expected planetary equilibrium temperature (390\u2013412\u2009K versus 160\u2009K). On the basis of cooling models, these results indicate that WD\u20091856\u2009b underwent a migration-related reheating event 3.0\u20135.5\u2009Gyr into the white dwarf phase, consistent with post-main-sequence tidal evolution to the present-day 0.02-\n                    <jats:sc>au<\/jats:sc>\n                    circular orbit. Our results provide a window into the ultimate fate of giant planets orbiting stars with masses similar to our Sun.\n                  <\/jats:p>","DOI":"10.1038\/s41586-026-10514-7","type":"journal-article","created":{"date-parts":[[2026,7,1]],"date-time":"2026-07-01T15:47:49Z","timestamp":1782920869000},"page":"76-80","update-policy":"https:\/\/doi.org\/10.1007\/springer_crossmark_policy","source":"Crossref","is-referenced-by-count":3,"title":["Aerosols and hydrocarbons in the atmosphere of a white dwarf planet"],"prefix":"10.1038","volume":"655","author":[{"ORCID":"https:\/\/orcid.org\/0000-0003-4816-3469","authenticated-orcid":false,"given":"Ryan J.","family":"MacDonald","sequence":"first","affiliation":[],"role":[{"vocabulary":"crossref","role":"author"}]},{"given":"Christopher E.","family":"O\u2019Connor","sequence":"additional","affiliation":[],"role":[{"vocabulary":"crossref","role":"author"}]},{"given":"Victoria A.","family":"Boehm","sequence":"additional","affiliation":[],"role":[{"vocabulary":"crossref","role":"author"}]},{"ORCID":"https:\/\/orcid.org\/0000-0002-2739-1465","authenticated-orcid":false,"given":"E. 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