{"id":21256,"date":"2026-08-28T18:10:54","date_gmt":"2026-08-28T18:10:54","guid":{"rendered":"https:\/\/www.radionet-org.eu\/radionet\/?p=21256"},"modified":"2026-08-28T18:10:54","modified_gmt":"2026-08-28T18:10:54","slug":"alma-reveals-a-trillion-mile-gas-stream-feeding-gw-orionis","status":"publish","type":"post","link":"https:\/\/www.radionet-org.eu\/radionet\/alma-reveals-a-trillion-mile-gas-stream-feeding-gw-orionis\/","title":{"rendered":"ALMA Reveals a Trillion-Mile Gas Stream Feeding GW Orionis"},"content":{"rendered":"<p>ALMA has captured a vast stream of gas feeding the young triple-star system GW Orionis, located about 1,300 light-years away. Stretching roughly 12,000 astronomical units (0.2 light-years), the streamer connects the surrounding molecular cloud with the system\u2019s unusual, misaligned planet-forming rings.<\/p>\n<p class=\"isSelectedEnd\">The observations provide strong evidence that late infall of material from a star\u2019s natal cloud can transfer angular momentum to a protoplanetary disk and influence its structure and evolution. The study combines observations from all three ALMA arrays and offers new insights into the dynamic environments in which planets form.<\/p>\n<p>For further details, see the <span class=\"text-token-text-primary cursor-text rounded-sm\"><a href=\"https:\/\/www.almaobservatory.org\/en\/press-releases\/alma-captures-a-trillion-mile-stream-feeding-the-triple-star-system-gw-orionis\/\">ALMA press release<\/a><\/span>\u00a0and the publication in <em>The Astronomical Journal (<a href=\"http:\/\/10.3847\/1538-3881\/ae8bae\">DOI<\/a>)<\/em>.<\/p>\n<p><span style=\"color: #333333\"><em>Credit- Image &#8211;\u00a0Artist\u2019s impression of a gas streamer feeding material onto the protoplanetary disk around GW Orionis and contributing to its misaligned dust rings. Credit:\u00a0NSF\/AUI\/NSF NRAO\/B. Saxton<\/em><\/span><\/p>\n","protected":false},"excerpt":{"rendered":"<p>ALMA has captured a vast stream of gas feeding the young triple-star system GW Orionis, located about 1,300 light-years away. Stretching roughly 12,000 astronomical units (0.2 light-years), the streamer connects the surrounding molecular cloud with the system\u2019s unusual, misaligned planet-forming rings. The observations provide strong evidence that late infall of material from a star\u2019s natal [&hellip;]<\/p>\n","protected":false},"author":24,"featured_media":21257,"comment_status":"closed","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":[],"categories":[118,9],"tags":[],"_links":{"self":[{"href":"https:\/\/www.radionet-org.eu\/radionet\/wp-json\/wp\/v2\/posts\/21256"}],"collection":[{"href":"https:\/\/www.radionet-org.eu\/radionet\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.radionet-org.eu\/radionet\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/www.radionet-org.eu\/radionet\/wp-json\/wp\/v2\/users\/24"}],"replies":[{"embeddable":true,"href":"https:\/\/www.radionet-org.eu\/radionet\/wp-json\/wp\/v2\/comments?post=21256"}],"version-history":[{"count":1,"href":"https:\/\/www.radionet-org.eu\/radionet\/wp-json\/wp\/v2\/posts\/21256\/revisions"}],"predecessor-version":[{"id":21258,"href":"https:\/\/www.radionet-org.eu\/radionet\/wp-json\/wp\/v2\/posts\/21256\/revisions\/21258"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/www.radionet-org.eu\/radionet\/wp-json\/wp\/v2\/media\/21257"}],"wp:attachment":[{"href":"https:\/\/www.radionet-org.eu\/radionet\/wp-json\/wp\/v2\/media?parent=21256"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.radionet-org.eu\/radionet\/wp-json\/wp\/v2\/categories?post=21256"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.radionet-org.eu\/radionet\/wp-json\/wp\/v2\/tags?post=21256"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}