{"id":239074,"date":"2025-11-02T05:40:07","date_gmt":"2025-11-02T05:40:07","guid":{"rendered":"https:\/\/www.newsbeep.com\/uk\/239074\/"},"modified":"2025-11-02T05:40:07","modified_gmt":"2025-11-02T05:40:07","slug":"nasas-voyager-spacecraft-found-a-30000-50000-kelvin-wall-at-the-edge-of-our-solar-system","status":"publish","type":"post","link":"https:\/\/www.newsbeep.com\/uk\/239074\/","title":{"rendered":"NASA&#8217;s Voyager Spacecraft Found A 30,000-50,000 Kelvin &#8220;Wall&#8221; At The Edge Of Our Solar System"},"content":{"rendered":"<p>In 1977, NASA launched the Voyager probes to explore the outer reaches of the Solar System and the interstellar space beyond. Eventually, both spacecraft encountered a blazing \u201cwall of fire\u201d at the system\u2019s boundary, recording temperatures between 30,000 and 50,000 kelvin (about 54,000 to 90,000 degrees Fahrenheit) as they passed through.<\/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;\" data-pasted=\"true\">There are a few ways you could define the edge of the Solar System \u2013 for instance, where the planets end, or at the Oort cloud, the boundary of the Sun&#8217;s gravitational influence, where objects may still\u00a0<a href=\"https:\/\/science.nasa.gov\/solar-system\/solar-system-facts\/#:~:text=The%20Oort%20Cloud%20is%20the,t%20extend%20quite%20as%20far.\" target=\"_blank\" rel=\"noopener noreferrer nofollow\" style=\"box-sizing: border-box; text-decoration-skip-ink: auto; color: rgb(104, 127, 30); text-decoration: underline;\">return closer<\/a> to the Sun. One way is to define it as the edge of the Sun&#8217;s magnetic field, where it pushes up against the interstellar medium, known as the heliopause.<\/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 nofollow\" 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;\">It is beyond that where the heliopause lies.<\/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 boundary between solar wind and interstellar wind is the heliopause, where the pressure of the two winds are in balance. This balance in pressure causes the solar wind to turn back and flow down the tail of the heliosphere,&#8221; NASA <a href=\"https:\/\/www.nasa.gov\/image-article\/heliosphere-4\/\" target=\"_blank\" rel=\"noopener noreferrer nofollow\" style=\"box-sizing: border-box; text-decoration-skip-ink: auto; color: rgb(104, 127, 30); text-decoration: underline;\">continues<\/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;\">\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;As the heliosphere plows through interstellar space, a <a href=\"https:\/\/www.iflscience.com\/these-galactic-clusters-smashed-into-each-other-giant-bow-shocks-suggest-theyre-about-to-go-for-round-2-79538\" target=\"_blank\" rel=\"noopener noreferrer nofollow\" style=\"box-sizing: border-box; text-decoration-skip-ink: auto; color: rgb(104, 127, 30); text-decoration: underline;\">bow shock<\/a> forms, similar to what forms as a ship plowing through the ocean.&#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;\" data-pasted=\"true\">On August 25, 2012, Voyager 1 became the first spacecraft to go beyond the heliosphere and cross the heliopause, followed by Voyager 2 in\u00a0<a href=\"https:\/\/www.iflscience.com\/voyager-2-has-just-entered-interstellar-space-nasa-confirms-50893\" target=\"_blank\" rel=\"noopener noreferrer nofollow\" style=\"box-sizing: border-box; text-decoration-skip-ink: auto; color: rgb(104, 127, 30); text-decoration: underline;\">2018<\/a>. Prior to the Voyager spacecraft crossing the heliopause, scientists didn&#8217;t really know where the boundary would be, but the fact that the probes hit it at different distances helped support a few predictions about it.<\/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;Scientists expected that the edge of the heliosphere, called the heliopause, can move as the Sun&#8217;s activity changes, sort of like a lung expanding and contracting with breath,&#8221; a\u00a0<a href=\"https:\/\/www.jpl.nasa.gov\/news\/voyager-2-illuminates-boundary-of-interstellar-space\/\" target=\"_blank\" rel=\"noopener noreferrer nofollow\" style=\"box-sizing: border-box; text-decoration-skip-ink: auto; color: rgb(104, 127, 30); text-decoration: underline;\">NASA statement<\/a> explains. &#8220;This was consistent with the fact that the two probes encountered the heliopause at different distances from the Sun.&#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;\">While not a hard edge, or a &#8220;wall&#8221; as it has sometimes been called, here both spacecraft measured temperatures of 30,000-50,000 kelvin (54,000-90,000 degrees Fahrenheit), which is why it is sometimes also referred to as a &#8220;<a href=\"https:\/\/www.iflscience.com\/why-some-people-call-the-solar-systems-edge-the-wall-of-fire-72918\" target=\"_blank\" rel=\"noopener noreferrer nofollow\" style=\"box-sizing: border-box; text-decoration-skip-ink: auto; color: rgb(104, 127, 30); text-decoration: underline;\">wall of fire<\/a>&#8220;. \u00a0The craft survived the wall as, though the particles they measured were extremely energetic, the chances of collision in this particle-sparse region of space are so low that not enough heat could be transferred to the duo.\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\u00a0<a href=\"https:\/\/www.iflscience.com\/tags\/voyager\" target=\"_blank\" rel=\"noopener noreferrer nofollow\" style=\"box-sizing: border-box; text-decoration-skip-ink: auto; color: rgb(104, 127, 30); text-decoration: underline;\">Voyager<\/a> spacecraft continue to send us data from beyond this &#8220;wall&#8221;, the only two probes that have crossed it so far, nearly 50 years after they were launched. Together, they have found several surprises on our first glimpse outside the Solar System.<\/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;An observation by Voyager 2&#8217;s magnetic field instrument confirms a surprising result from Voyager 1: The magnetic field in the region just beyond the heliopause is parallel to the magnetic field inside the heliosphere,&#8221; NASA explained, shortly after one such surprise.\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;\">&#8220;With Voyager 1, scientists had only one sample of these magnetic fields and couldn&#8217;t say for sure whether the apparent alignment was characteristic of the entire exterior region or just a coincidence. Voyager 2&#8217;s magnetometer observations confirm the Voyager 1 finding and indicate that the two fields align.&#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;\">An earlier version of this <a href=\"https:\/\/www.iflscience.com\/nasas-voyager-spacecraft-found-a-30000-50000-kelvin-wall-at-the-edge-of-our-solar-system-79454\" target=\"_blank\" rel=\"noopener noreferrer nofollow\">article<\/a> appeared in June.<\/p>\n","protected":false},"excerpt":{"rendered":"In 1977, NASA launched the Voyager probes to explore the outer reaches of the Solar System and the&hellip;\n","protected":false},"author":2,"featured_media":239075,"comment_status":"","ping_status":"","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[23],"tags":[90,416,56,54,55],"class_list":{"0":"post-239074","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","12":"tag-unitedkingdom"},"_links":{"self":[{"href":"https:\/\/www.newsbeep.com\/uk\/wp-json\/wp\/v2\/posts\/239074","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.newsbeep.com\/uk\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.newsbeep.com\/uk\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/www.newsbeep.com\/uk\/wp-json\/wp\/v2\/users\/2"}],"replies":[{"embeddable":true,"href":"https:\/\/www.newsbeep.com\/uk\/wp-json\/wp\/v2\/comments?post=239074"}],"version-history":[{"count":0,"href":"https:\/\/www.newsbeep.com\/uk\/wp-json\/wp\/v2\/posts\/239074\/revisions"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/www.newsbeep.com\/uk\/wp-json\/wp\/v2\/media\/239075"}],"wp:attachment":[{"href":"https:\/\/www.newsbeep.com\/uk\/wp-json\/wp\/v2\/media?parent=239074"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.newsbeep.com\/uk\/wp-json\/wp\/v2\/categories?post=239074"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.newsbeep.com\/uk\/wp-json\/wp\/v2\/tags?post=239074"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}