{"id":327341,"date":"2025-08-08T07:49:09","date_gmt":"2025-08-08T07:49:09","guid":{"rendered":"https:\/\/www.europesays.com\/uk\/327341\/"},"modified":"2025-08-08T07:49:09","modified_gmt":"2025-08-08T07:49:09","slug":"an-encounter-with-something-from-outside-our-solar-system-may-have-cooled-earth-in-a-big-way","status":"publish","type":"post","link":"https:\/\/www.europesays.com\/uk\/327341\/","title":{"rendered":"An &#8220;Encounter&#8221; With Something From Outside Our Solar System May Have Cooled Earth In A Big Way"},"content":{"rendered":"<p>As the Moon orbits the Earth, and the Earth circles the Sun, the Sun itself travels around the center of the Milky Way\u2014rising and falling above and below the galaxy\u2019s plane along the way.<\/p>\n<p style=\"box-sizing: border-box; margin: 0px 0px 1.5rem; font-weight: 400; line-height: 1.75; letter-spacing: 0.5px; color: rgb(0, 0, 0); font-family: Karla, sans-serif; font-size: medium; font-style: normal; font-variant-ligatures: normal; font-variant-caps: normal; orphans: 2; text-align: start; text-indent: 0px; text-transform: none; widows: 2; word-spacing: 0px; -webkit-text-stroke-width: 0px; white-space: normal; background-color: rgb(255, 255, 255); text-decoration-thickness: initial; text-decoration-style: initial; text-decoration-color: initial;\" id=\"isPasted\">A study has suggested that this motion of our star through the galaxy potentially takes us through regions of space that could affect our planet&#8217;s climate. According to the study, the Solar System may have passed through an interstellar cloud so dense that it may have interfered with the flow of the solar wind, potentially cooling the planets.\u00a0<\/p>\n<p style=\"box-sizing: border-box; margin: 0px 0px 1.5rem; font-weight: 400; line-height: 1.75; letter-spacing: 0.5px; color: rgb(0, 0, 0); font-family: Karla, sans-serif; font-size: medium; font-style: normal; font-variant-ligatures: normal; font-variant-caps: normal; orphans: 2; text-align: start; text-indent: 0px; text-transform: none; widows: 2; word-spacing: 0px; -webkit-text-stroke-width: 0px; white-space: normal; background-color: rgb(255, 255, 255); text-decoration-thickness: initial; text-decoration-style: initial; text-decoration-color: initial;\">The Solar System is protected, to some extent, from the interstellar medium (ISM) by our <a href=\"https:\/\/www.iflscience.com\/there-are-ripples-at-the-boundary-of-interstellar-space-65753\" target=\"_blank\" rel=\"noopener noreferrer\" style=\"box-sizing: border-box; text-decoration-skip-ink: auto; color: rgb(104, 127, 30); text-decoration: underline;\">heliosphere<\/a>.<\/p>\n<p style=\"box-sizing: border-box; margin: 0px 0px 1.5rem; font-weight: 400; line-height: 1.75; letter-spacing: 0.5px; color: rgb(0, 0, 0); font-family: Karla, sans-serif; font-size: medium; font-style: normal; font-variant-ligatures: normal; font-variant-caps: normal; orphans: 2; text-align: start; text-indent: 0px; text-transform: none; widows: 2; word-spacing: 0px; -webkit-text-stroke-width: 0px; white-space: normal; background-color: rgb(255, 255, 255); text-decoration-thickness: initial; text-decoration-style: initial; text-decoration-color: initial;\">&#8220;The Sun sends out a constant flow of charged particles called the solar wind, which ultimately travels past all the planets to some three times the distance to Pluto before being impeded by the interstellar medium,&#8221; <a href=\"https:\/\/science.nasa.gov\/heliophysics\/focus-areas\/heliosphere\/\" target=\"_blank\" rel=\"noopener noreferrer\" style=\"box-sizing: border-box; text-decoration-skip-ink: auto; color: rgb(104, 127, 30); text-decoration: underline;\">NASA explains<\/a>. &#8220;This forms a giant bubble around the Sun and its planets, known as the heliosphere.&#8221;<\/p>\n<p style=\"box-sizing: border-box; margin: 0px 0px 1.5rem; font-weight: 400; line-height: 1.75; letter-spacing: 0.5px; color: rgb(0, 0, 0); font-family: Karla, sans-serif; font-size: medium; font-style: normal; font-variant-ligatures: normal; font-variant-caps: normal; orphans: 2; text-align: start; text-indent: 0px; text-transform: none; widows: 2; word-spacing: 0px; -webkit-text-stroke-width: 0px; white-space: normal; background-color: rgb(255, 255, 255); text-decoration-thickness: initial; text-decoration-style: initial; text-decoration-color: initial;\">The Solar System is currently in a 1,000-light-year-wide &#8220;<a href=\"https:\/\/www.iflscience.com\/we-live-inside-a-1-000-light-year-wide-bubble-whose-magnetism-has-been-mapped-67059\" target=\"_blank\" rel=\"noopener noreferrer\" style=\"box-sizing: border-box; text-decoration-skip-ink: auto; color: rgb(104, 127, 30); text-decoration: underline; font-family: Karla, sans-serif; font-size: medium; font-style: normal; font-variant-ligatures: normal; font-variant-caps: normal; font-weight: 400; letter-spacing: 0.5px; orphans: 2; text-align: start; text-indent: 0px; text-transform: none; widows: 2; word-spacing: 0px; -webkit-text-stroke-width: 0px; white-space: normal; background-color: rgb(255, 255, 255);\">Local Bubble<\/a>&#8220;, or &#8220;local interstellar cloud&#8221; (LIC). This &#8220;bubble&#8221; is a lot less dense than typical interstellar space, with 0.001 particles per cubic centimeter compared to the typical\u00a0<a href=\"http:\/\/www-ssg.sr.unh.edu\/ism\/LISM.html#:~:text=Our%20local%20cloud%2C%20which%20features,1%2C000%2C000%20K).\" target=\"_blank\" rel=\"noopener noreferrer\" style=\"box-sizing: border-box; text-decoration-skip-ink: auto; color: rgb(104, 127, 30); text-decoration: underline; font-family: Karla, sans-serif; font-size: medium; font-style: normal; font-variant-ligatures: normal; font-variant-caps: normal; font-weight: 400; letter-spacing: 0.5px; orphans: 2; text-align: start; text-indent: 0px; text-transform: none; widows: 2; word-spacing: 0px; -webkit-text-stroke-width: 0px; white-space: normal; background-color: rgb(255, 255, 255);\">0.1 atoms per cubic centimeter<\/a>. The Solar System will leave this sparse region of space in the next few thousand years and head once more into the interstellar medium.<\/p>\n<p style=\"box-sizing: border-box; margin: 0px 0px 1.5rem; font-weight: 400; line-height: 1.75; letter-spacing: 0.5px; color: rgb(0, 0, 0); font-family: Karla, sans-serif; font-size: medium; font-style: normal; font-variant-ligatures: normal; font-variant-caps: normal; orphans: 2; text-align: start; text-indent: 0px; text-transform: none; widows: 2; word-spacing: 0px; -webkit-text-stroke-width: 0px; white-space: normal; background-color: rgb(255, 255, 255); text-decoration-thickness: initial; text-decoration-style: initial; text-decoration-color: initial;\">\n<p style=\"box-sizing: border-box; margin: 0px 0px 1.5rem; font-weight: 400; line-height: 1.75; letter-spacing: 0.5px; color: rgb(0, 0, 0); font-family: Karla, sans-serif; font-size: medium; font-style: normal; font-variant-ligatures: normal; font-variant-caps: normal; orphans: 2; text-align: start; text-indent: 0px; text-transform: none; widows: 2; word-spacing: 0px; -webkit-text-stroke-width: 0px; white-space: normal; background-color: rgb(255, 255, 255); text-decoration-thickness: initial; text-decoration-style: initial; text-decoration-color: initial;\" id=\"isPasted\">Looking at the Solar System&#8217;s path, and mapping the Local Ribbon of Cold Clouds, the team found we have likely traveled through denser regions in the past.<\/p>\n<p style=\"box-sizing: border-box; margin: 0px 0px 1.5rem; font-weight: 400; line-height: 1.75; letter-spacing: 0.5px; color: rgb(0, 0, 0); font-family: Karla, sans-serif; font-size: medium; font-style: normal; font-variant-ligatures: normal; font-variant-caps: normal; orphans: 2; text-align: start; text-indent: 0px; text-transform: none; widows: 2; word-spacing: 0px; -webkit-text-stroke-width: 0px; white-space: normal; background-color: rgb(255, 255, 255); text-decoration-thickness: initial; text-decoration-style: initial; text-decoration-color: initial;\">&#8220;In the ISM that the Sun has traversed for the last couple of million years, there are cold, compact clouds that could have drastically affected the heliosphere,&#8221; the team explains in their paper. &#8220;We explore a scenario whereby the Solar System went through a cold gas cloud a few million years ago.&#8221;<\/p>\n<p style=\"box-sizing: border-box; margin: 0px 0px 1.5rem; font-weight: 400; line-height: 1.75; letter-spacing: 0.5px; color: rgb(0, 0, 0); font-family: Karla, sans-serif; font-size: medium; font-style: normal; font-variant-ligatures: normal; font-variant-caps: normal; orphans: 2; text-align: start; text-indent: 0px; text-transform: none; widows: 2; word-spacing: 0px; -webkit-text-stroke-width: 0px; white-space: normal; background-color: rgb(255, 255, 255); text-decoration-thickness: initial; text-decoration-style: initial; text-decoration-color: initial;\">Though research on the effects of traversing such regions has been sparser than atoms in the local bubble, the team believes it could have contracted our heliosphere, which in turn had an effect on our climate. Our heliosphere is protective, and as it contracted some of the material in these denser regions could reach Earth.<\/p>\n<p style=\"box-sizing: border-box; margin: 0px 0px 1.5rem; font-weight: 400; line-height: 1.75; letter-spacing: 0.5px; color: rgb(0, 0, 0); font-family: Karla, sans-serif; font-size: medium; font-style: normal; font-variant-ligatures: normal; font-variant-caps: normal; orphans: 2; text-align: start; text-indent: 0px; text-transform: none; widows: 2; word-spacing: 0px; -webkit-text-stroke-width: 0px; white-space: normal; background-color: rgb(255, 255, 255); text-decoration-thickness: initial; text-decoration-style: initial; text-decoration-color: initial;\">&#8220;Large amounts of neutral hydrogen as a result of an encounter with cold clouds with densities above 1,000\u2009cm\u22123 will alter the chemistry of Earth\u2019s atmosphere,&#8221; the team wrote. &#8220;Very few works have investigated the climatic effects of such encounters quantitatively in the context of encounters with dense giant molecular clouds. Some argue that such high densities would deplete the ozone in the mid-atmosphere (50\u2013100\u2009km [31\u201362 miles]) and eventually cool the Earth.&#8221;<\/p>\n<p style=\"box-sizing: border-box; margin: 0px 0px 1.5rem; font-weight: 400; line-height: 1.75; letter-spacing: 0.5px; color: rgb(0, 0, 0); font-family: Karla, sans-serif; font-size: medium; font-style: normal; font-variant-ligatures: normal; font-variant-caps: normal; orphans: 2; text-align: start; text-indent: 0px; text-transform: none; widows: 2; word-spacing: 0px; -webkit-text-stroke-width: 0px; white-space: normal; background-color: rgb(255, 255, 255); text-decoration-thickness: initial; text-decoration-style: initial; text-decoration-color: initial;\">The team says that geological evidence of increased amounts of 60Fe (iron 60) and 244Pu (plutonium 244) isotopes found in ice cores, the oceans, Antarctic snow, and samples of the Moon, could be evidence of these particles reaching Earth as we traversed the Local Lynx of Cold Cloud 2\u2009million years ago.\u00a0<\/p>\n<p style=\"box-sizing: border-box; margin: 0px 0px 1.5rem; font-weight: 400; line-height: 1.75; letter-spacing: 0.5px; color: rgb(0, 0, 0); font-family: Karla, sans-serif; font-size: medium; font-style: normal; font-variant-ligatures: normal; font-variant-caps: normal; orphans: 2; text-align: start; text-indent: 0px; text-transform: none; widows: 2; word-spacing: 0px; -webkit-text-stroke-width: 0px; white-space: normal; background-color: rgb(255, 255, 255); text-decoration-thickness: initial; text-decoration-style: initial; text-decoration-color: initial;\">These isotopes are spat out by supernovas and neutron star mergers, which then become trapped by interstellar dust. These isotopes in the geological record have previously been explained as being sent here by a close supernova, but the current team believes they could be explained better by particles trapped in the cloud, as a close-by supernova would collapse the heliosphere to distances of 1 AU (the distance between the Earth and the Sun), while a further afield supernova would not deposit enough 60Fe on Earth.<\/p>\n<p style=\"box-sizing: border-box; margin: 0px 0px 1.5rem; font-weight: 400; line-height: 1.75; letter-spacing: 0.5px; color: rgb(0, 0, 0); font-family: Karla, sans-serif; font-size: medium; font-style: normal; font-variant-ligatures: normal; font-variant-caps: normal; orphans: 2; text-align: start; text-indent: 0px; text-transform: none; widows: 2; word-spacing: 0px; -webkit-text-stroke-width: 0px; white-space: normal; background-color: rgb(255, 255, 255); text-decoration-thickness: initial; text-decoration-style: initial; text-decoration-color: initial;\">\u201cThis paper is the first to quantitatively show there was an encounter between the Sun and something outside of the solar system that would have affected Earth\u2019s climate,\u201d space physicist at Boston University, Merav Opher, said in a <a href=\"https:\/\/www.bu.edu\/articles\/2024\/the-solar-system-may-have-passed-through-interstellar-clouds\/\" target=\"_blank\" rel=\"noopener noreferrer\" style=\"box-sizing: border-box; text-decoration-skip-ink: auto; color: rgb(104, 127, 30); text-decoration: underline;\">statement<\/a>, later adding, &#8220;but as soon as the Earth was away from the cold cloud, the heliosphere engulfed all the planets, including Earth.&#8221;<\/p>\n<p style=\"box-sizing: border-box; margin: 0px 0px 1.5rem; font-weight: 400; line-height: 1.75; letter-spacing: 0.5px; color: rgb(0, 0, 0); font-family: Karla, sans-serif; font-size: medium; font-style: normal; font-variant-ligatures: normal; font-variant-caps: normal; orphans: 2; text-align: start; text-indent: 0px; text-transform: none; widows: 2; word-spacing: 0px; -webkit-text-stroke-width: 0px; white-space: normal; background-color: rgb(255, 255, 255); text-decoration-thickness: initial; text-decoration-style: initial; text-decoration-color: initial;\">The contraction of the heliosphere could have lasted from hundreds of years to a million years, according to the team, and it is likely we will encounter another such heliosphere-contracting cloud within another million years or so.\u00a0<\/p>\n<p style=\"box-sizing: border-box; margin: 0px 0px 1.5rem; font-weight: 400; line-height: 1.75; letter-spacing: 0.5px; color: rgb(0, 0, 0); font-family: Karla, sans-serif; font-size: medium; font-style: normal; font-variant-ligatures: normal; font-variant-caps: normal; orphans: 2; text-align: start; text-indent: 0px; text-transform: none; widows: 2; word-spacing: 0px; -webkit-text-stroke-width: 0px; white-space: normal; background-color: rgb(255, 255, 255); text-decoration-thickness: initial; text-decoration-style: initial; text-decoration-color: initial;\">While interesting, there is a lot more to find out.<\/p>\n<p style=\"box-sizing: border-box; margin: 0px 0px 1.5rem; font-weight: 400; line-height: 1.75; letter-spacing: 0.5px; color: rgb(0, 0, 0); font-family: Karla, sans-serif; font-size: medium; font-style: normal; font-variant-ligatures: normal; font-variant-caps: normal; orphans: 2; text-align: start; text-indent: 0px; text-transform: none; widows: 2; word-spacing: 0px; -webkit-text-stroke-width: 0px; white-space: normal; background-color: rgb(255, 255, 255); text-decoration-thickness: initial; text-decoration-style: initial; text-decoration-color: initial;\">&#8220;This work should be revisited with modern atmospheric modelling,&#8221; the team writes. &#8220;It has been suggested that climate changes around this time could have affected human evolution. The hypothesis is that the emergence of our species Homo sapiens was shaped by the need to adapt to climate change. With the shrinkage of the heliosphere, the Earth was exposed directly to the ISM.&#8221;<\/p>\n<p style=\"box-sizing: border-box; margin: 0px 0px 1.5rem; font-weight: 400; line-height: 1.75; letter-spacing: 0.5px; color: rgb(0, 0, 0); font-family: Karla, sans-serif; font-size: medium; font-style: normal; font-variant-ligatures: normal; font-variant-caps: normal; orphans: 2; text-align: start; text-indent: 0px; text-transform: none; widows: 2; word-spacing: 0px; -webkit-text-stroke-width: 0px; white-space: normal; background-color: rgb(255, 255, 255); text-decoration-thickness: initial; text-decoration-style: initial; text-decoration-color: initial;\">The paper was published in <a href=\"https:\/\/www.nature.com\/articles\/s41550-024-02279-8\" target=\"_blank\" rel=\"noopener noreferrer\" style=\"box-sizing: border-box; text-decoration-skip-ink: auto; color: rgb(104, 127, 30); text-decoration: underline;\">Nature Astronomy<\/a>.<\/p>\n<p style=\"box-sizing: border-box; margin: 0px 0px 1.5rem; font-weight: 400; line-height: 1.75; letter-spacing: 0.5px; color: rgb(0, 0, 0); font-family: Karla, sans-serif; font-size: medium; font-style: normal; font-variant-ligatures: normal; font-variant-caps: normal; orphans: 2; text-align: start; text-indent: 0px; text-transform: none; widows: 2; word-spacing: 0px; -webkit-text-stroke-width: 0px; white-space: normal; background-color: rgb(255, 255, 255); text-decoration-thickness: initial; text-decoration-style: initial; text-decoration-color: initial;\">An earlier version of this story was\u00a0<a href=\"https:\/\/www.iflscience.com\/encounter-between-sun-and-something-outside-the-solar-system-may-have-dramatically-cooled-earth-74635\" target=\"_blank\" rel=\"noopener noreferrer\">published<\/a>\u00a0in 2024.<\/p>\n","protected":false},"excerpt":{"rendered":"As the Moon orbits the Earth, and the Earth circles the Sun, the Sun itself travels around the&hellip;\n","protected":false},"author":2,"featured_media":327342,"comment_status":"","ping_status":"","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[3844],"tags":[70,413,16,15],"class_list":{"0":"post-327341","1":"post","2":"type-post","3":"status-publish","4":"format-standard","5":"has-post-thumbnail","7":"category-space","8":"tag-science","9":"tag-space","10":"tag-uk","11":"tag-united-kingdom"},"share_on_mastodon":{"url":"","error":""},"_links":{"self":[{"href":"https:\/\/www.europesays.com\/uk\/wp-json\/wp\/v2\/posts\/327341","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.europesays.com\/uk\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.europesays.com\/uk\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/www.europesays.com\/uk\/wp-json\/wp\/v2\/users\/2"}],"replies":[{"embeddable":true,"href":"https:\/\/www.europesays.com\/uk\/wp-json\/wp\/v2\/comments?post=327341"}],"version-history":[{"count":0,"href":"https:\/\/www.europesays.com\/uk\/wp-json\/wp\/v2\/posts\/327341\/revisions"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/www.europesays.com\/uk\/wp-json\/wp\/v2\/media\/327342"}],"wp:attachment":[{"href":"https:\/\/www.europesays.com\/uk\/wp-json\/wp\/v2\/media?parent=327341"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.europesays.com\/uk\/wp-json\/wp\/v2\/categories?post=327341"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.europesays.com\/uk\/wp-json\/wp\/v2\/tags?post=327341"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}