{"id":398184,"date":"2026-03-22T13:21:13","date_gmt":"2026-03-22T13:21:13","guid":{"rendered":"https:\/\/www.europesays.com\/ie\/398184\/"},"modified":"2026-03-22T13:21:13","modified_gmt":"2026-03-22T13:21:13","slug":"hydrogen-atmospheres-keep-rogue-moons-warm-for-billions-of-years","status":"publish","type":"post","link":"https:\/\/www.europesays.com\/ie\/398184\/","title":{"rendered":"Hydrogen atmospheres keep rogue moons warm for billions of years"},"content":{"rendered":"<p>A new study led by researchers at the Max Planck Institute for Extraterrestrial Physics and Giulia Roccetti of the European Space Agency suggests rogue planets may host habitable moons. <\/p>\n<p>The team found that thick hydrogen atmospheres can trap tidal heat, keeping surfaces warm enough for liquid water for up to 4.3 billion years. <\/p>\n<p>Unlike CO\u2082-based models, these atmospheres avoid collapse. Combined with tidal-driven wet\u2013dry cycles and ammonia-rich chemistry, such environments could support early life processes\u2014even without any starlight.<\/p>\n<p>\u201cWe find that such atmospheres can effectively trap heat via collision-induced absorption of H2, maintaining surface temperatures suitable for liquid water for time-scales of up to 4.3 Gyr, depending on the surface pressure, while not prone to condensation-induced collapse,\u201d said researchers in the study abstract. <\/p>\n<p>Rogue moon habitats<\/p>\n<p>Astronomers have identified hundreds of exoplanets drifting through interstellar space, many likely ejected from their parent systems by past gravitational interactions. <\/p>\n<p>While these rogue planets are expected to be cold and dark, their moons may follow a different path. During ejection, a moon\u2019s orbit can become highly elongated, generating strong tidal forces as it is repeatedly stretched and compressed by its host planet. Similar to Europa and Enceladus, this process can produce significant internal heat, reports Phys.org. <\/p>\n<p>If a moon\u2019s atmosphere allows gases to condense, much of this heat would escape into space. However, in dense, hydrogen-dominated atmospheres, heat retention can increase. Under high pressure, hydrogen molecules absorb infrared radiation through collision-induced absorption, where temporary molecular complexes form during collisions.<\/p>\n<p>These complexes enhance heat absorption, comparable to greenhouse gases like carbon dioxide and methane. As a result, internal heat could be trapped efficiently without atmospheric collapse. Researchers say such moons could maintain surface temperatures high enough for liquid water without requiring energy from a nearby star, although detecting and analysing such atmospheres remains challenging.<\/p>\n<p>Hidden ocean worlds<\/p>\n<p>The new study suggests that <a href=\"https:\/\/interestingengineering.com\/space\/spacex-readies-worlds-most-powerful-rocket\" id=\"https:\/\/interestingengineering.com\/space\/spacex-readies-worlds-most-powerful-rocket\" target=\"_blank\" rel=\"dofollow noopener\">moons<\/a> orbiting rogue <a href=\"https:\/\/interestingengineering.com\/space\/discovery-breaks-the-rule-of-planet-formation\" id=\"https:\/\/interestingengineering.com\/space\/discovery-breaks-the-rule-of-planet-formation\" target=\"_blank\" rel=\"dofollow noopener\">exoplanets<\/a> could sustain habitable conditions for billions of years\u2014despite the absence of any nearby star. The research highlights the role of dense, hydrogen-rich atmospheres in trapping internal heat.<\/p>\n<p>Using advanced simulations, the team modeled how a moon\u2019s orbit and atmosphere evolve after its host planet is ejected into interstellar space. Their approach combined atmospheric temperature calculations with chemical processes such as condensation, alongside updated models of orbital evolution that account for declining tidal heating over time.<\/p>\n<p>Rogue planets\u2014many of which have already been detected drifting through space\u2014are thought to have been expelled from their original systems through gravitational interactions. While these planets are expected to be extremely cold, their moons may experience intense tidal heating if their orbits become highly elongated. Similar processes are observed on Europa and Enceladus, where gravitational forces generate internal heat, reports <a href=\"https:\/\/phys.org\/news\/2026-03-moons-orbiting-exoplanets-habitable.html\" target=\"_blank\" rel=\"noopener noreferrer nofollow\">Phys.org<\/a>.<\/p>\n<p>The study finds that thick <a href=\"https:\/\/interestingengineering.com\/energy\/new-hydrogen-drone-addresses-range-limitations\" id=\"https:\/\/interestingengineering.com\/energy\/new-hydrogen-drone-addresses-range-limitations\" target=\"_blank\" rel=\"dofollow noopener\">hydrogen<\/a> atmospheres, potentially up to 100 times Earth\u2019s surface pressure, can efficiently trap this heat through collision-induced absorption. Under such conditions, temporary molecular interactions enhance infrared absorption, allowing heat to be retained far more effectively than in carbon dioxide\u2013dominated atmospheres, which are prone to collapse.<\/p>\n<p>As a result, some of these moons could maintain surface temperatures suitable for liquid water for up to 4.3 billion years. The presence of gases such as methane, ammonia, and water vapor may further stabilize these environments, significantly extending the potential window for habitability.<\/p>\n<p>\u201cWet-dry cycling caused by the strong tides together with the alkalinity of dissolved NH3\u00a0could create favourable conditions for RNA polymerisation and thus support the emergence of life,\u201d said the team in the research <a href=\"https:\/\/academic.oup.com\/mnras\/advance-article\/doi\/10.1093\/mnras\/stag243\/8496061?guestAccessKey=&amp;login=false\" id=\"https:\/\/academic.oup.com\/mnras\/advance-article\/doi\/10.1093\/mnras\/stag243\/8496061?guestAccessKey=&amp;login=false\" target=\"_blank\" rel=\"noopener noreferrer nofollow\">abstract<\/a>.<\/p>\n","protected":false},"excerpt":{"rendered":"A new study led by researchers at the Max Planck Institute for Extraterrestrial Physics and Giulia Roccetti of&hellip;\n","protected":false},"author":2,"featured_media":398185,"comment_status":"","ping_status":"","sticky":false,"template":"","format":"standard","meta":{"footnotes":"","_share_on_mastodon":"0"},"categories":[77],"tags":[160585,18,28434,60175,6123,8415,19,17,181006,10626,133,181007],"class_list":["post-398184","post","type-post","status-publish","format-standard","has-post-thumbnail","category-science","tag-alien-life","tag-eire","tag-european-space-agency","tag-exomoons","tag-exoplanets","tag-hydrogen","tag-ie","tag-ireland","tag-max-planck-institute-for-extraterrestrial-physics","tag-moon","tag-science","tag-space-life"],"share_on_mastodon":{"url":"https:\/\/pubeurope.com\/@ie\/116273039643782746","error":""},"_links":{"self":[{"href":"https:\/\/www.europesays.com\/ie\/wp-json\/wp\/v2\/posts\/398184","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.europesays.com\/ie\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.europesays.com\/ie\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/www.europesays.com\/ie\/wp-json\/wp\/v2\/users\/2"}],"replies":[{"embeddable":true,"href":"https:\/\/www.europesays.com\/ie\/wp-json\/wp\/v2\/comments?post=398184"}],"version-history":[{"count":0,"href":"https:\/\/www.europesays.com\/ie\/wp-json\/wp\/v2\/posts\/398184\/revisions"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/www.europesays.com\/ie\/wp-json\/wp\/v2\/media\/398185"}],"wp:attachment":[{"href":"https:\/\/www.europesays.com\/ie\/wp-json\/wp\/v2\/media?parent=398184"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.europesays.com\/ie\/wp-json\/wp\/v2\/categories?post=398184"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.europesays.com\/ie\/wp-json\/wp\/v2\/tags?post=398184"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}