{"id":618869,"date":"2023-03-17T09:48:55","date_gmt":"2023-03-17T14:48:55","guid":{"rendered":"https:\/\/news.sellorbuyhomefast.com\/index.php\/2023\/03\/17\/we-finally-have-proof-of-active-volcanoes-on-venus\/"},"modified":"2023-03-17T09:48:55","modified_gmt":"2023-03-17T14:48:55","slug":"we-finally-have-proof-of-active-volcanoes-on-venus","status":"publish","type":"post","link":"https:\/\/newsycanuse.com\/index.php\/2023\/03\/17\/we-finally-have-proof-of-active-volcanoes-on-venus\/","title":{"rendered":"We finally have proof of active volcanoes on Venus"},"content":{"rendered":"<div itemprop=\"articleBody\">\n<figure>\n  <img decoding=\"async\" src=\"https:\/\/cdn.arstechnica.net\/wp-content\/uploads\/2023\/03\/venus-list-800x394.jpg\" alt=\"Perspective view of Venusian volcano\"><figcaption>\n<p><a href=\"https:\/\/cdn.arstechnica.net\/wp-content\/uploads\/2023\/03\/venus-list.jpg\" data-height=\"668\" data-width=\"1356\">Enlarge<\/a> <span>\/<\/span> A perspective view across Maat Mons on Venus, based on Magellan radar data.<\/p>\n<p>NASA\/JPL<\/p>\n<\/figcaption><\/figure>\n<p>Venus is almost the same size, mass, and density as Earth. So it should be generating heat in its interior (by the decay of radioactive elements) at much the same rate as the Earth does. On Earth, one of the main ways in which this heat leaks out is via volcanic eruptions. During an average year, at least 50 volcanoes erupt.<\/p>\n<p>But despite decades of looking, we\u2019ve not seen clear signs of volcanic eruptions on Venus\u2014until now. A new study by geophysicist <a href=\"https:\/\/uaf.edu\/experts\/robert-herrick.php\">Robert Herrick<\/a> of the University of Alaska, Fairbanks, which he reported this week at the Lunar &#038; Planetary Science Conference in Houston and <a href=\"http:\/\/www.science.org\/doi\/10.1126\/science.abm7735\">published in the journal Science<\/a>, has at last caught one of the planet\u2019s volcanoes in the act.<\/p>\n<p>It\u2019s not straightforward to study Venus\u2019 surface because it has a dense atmosphere, including an unbroken cloud layer at a height of 45-65 km that is opaque to most wavelengths of radiation, including visible light. The only way to get a detailed view of the ground from above the clouds is by radar directed downward from an orbiting spacecraft.<\/p>\n<figure><a href=\"https:\/\/cdn.arstechnica.net\/wp-content\/uploads\/2023\/03\/venus-1.jpg\" data-height=\"1508\" data-width=\"1508\" alt=\"Venus seen in ultraviolet light by Japan\u2019s Akatsuki spacecraft in December 2016. The surface cannot be seen.\"><img loading=\"lazy\" decoding=\"async\" alt=\"Venus seen in ultraviolet light by Japan\u2019s Akatsuki spacecraft in December 2016. The surface cannot be seen.\" src=\"https:\/\/cdn.arstechnica.net\/wp-content\/uploads\/2023\/03\/venus-1-640x640.jpg\" width=\"640\" height=\"640\" ><\/a><figcaption>\n<p><a href=\"https:\/\/cdn.arstechnica.net\/wp-content\/uploads\/2023\/03\/venus-1.jpg\" data-height=\"1508\" data-width=\"1508\">Enlarge<\/a> <span>\/<\/span> Venus seen in ultraviolet light by Japan\u2019s Akatsuki spacecraft in December 2016. The surface cannot be seen.<\/p>\n<p>ISAS\/JAXA<\/p>\n<\/figcaption><\/figure>\n<p>A technique known as aperture synthesis is used to build up an image of the surface. This combines the varying strength of the radar echos bounced back from the ground\u2014including the time delay between transmission and receipt, plus slight shifts in frequency corresponding to whether the spacecraft is getting closer to or further from the origin of a particular echo. The resulting image looks rather like a black and white photograph, except that the brighter areas usually correspond to rougher surfaces and the darker areas to smoother surfaces.<\/p>\n<figure><a href=\"https:\/\/cdn.arstechnica.net\/wp-content\/uploads\/2023\/03\/venus-2.jpg\" data-height=\"926\" data-width=\"1508\" alt=\"140 km wide Magellan radar image of Venus showing lava flows (bright because they are rough) that have begun to encroach on an older impact crater.\"><img loading=\"lazy\" decoding=\"async\" alt=\"140 km wide Magellan radar image of Venus showing lava flows (bright because they are rough) that have begun to encroach on an older impact crater.\" src=\"https:\/\/cdn.arstechnica.net\/wp-content\/uploads\/2023\/03\/venus-2-640x393.jpg\" width=\"640\" height=\"393\" ><\/a><figcaption>\n<p><a href=\"https:\/\/cdn.arstechnica.net\/wp-content\/uploads\/2023\/03\/venus-2.jpg\" data-height=\"926\" data-width=\"1508\">Enlarge<\/a> <span>\/<\/span> 140 km wide Magellan radar image of Venus showing lava flows (bright because they are rough) that have begun to encroach on an older impact crater.<\/p>\n<p>NASA\/JPL<\/p>\n<\/figcaption><\/figure>\n<p>Nasa\u2019s Magellan probe orbited Venus from August 1990 to October 1994 and used this sort of radar technique to map the planet\u2019s surface with a spatial resolution of about a hundred meters at best. It showed that over 80 percent of the surface is covered by lava flows, but just how recently the youngest of them were erupted, and whether any eruptions continue today, remained a mystery for the next three decades.<\/p>\n<\/p><\/div>\n<p><a href=\"https:\/\/arstechnica.com\/?p=1924805\" class=\"button purchase\" rel=\"nofollow noopener\" target=\"_blank\">Read More<\/a><br \/>\n The Conversation<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Enlarge \/ A perspective view across Maat Mons on Venus, based on Magellan radar data.NASA\/JPL Venus is almost the same size, mass, and density as Earth. So it should be generating heat in its interior (by the decay of radioactive elements) at much the same rate as the Earth does. On Earth, one of the<\/p>\n","protected":false},"author":1,"featured_media":618870,"comment_status":"closed","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[848,2461,46],"tags":[],"class_list":{"0":"post-618869","1":"post","2":"type-post","3":"status-publish","4":"format-standard","5":"has-post-thumbnail","7":"category-finally","8":"category-proof","9":"category-technology"},"aioseo_notices":[],"_links":{"self":[{"href":"https:\/\/newsycanuse.com\/index.php\/wp-json\/wp\/v2\/posts\/618869","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/newsycanuse.com\/index.php\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/newsycanuse.com\/index.php\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/newsycanuse.com\/index.php\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/newsycanuse.com\/index.php\/wp-json\/wp\/v2\/comments?post=618869"}],"version-history":[{"count":0,"href":"https:\/\/newsycanuse.com\/index.php\/wp-json\/wp\/v2\/posts\/618869\/revisions"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/newsycanuse.com\/index.php\/wp-json\/wp\/v2\/media\/618870"}],"wp:attachment":[{"href":"https:\/\/newsycanuse.com\/index.php\/wp-json\/wp\/v2\/media?parent=618869"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/newsycanuse.com\/index.php\/wp-json\/wp\/v2\/categories?post=618869"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/newsycanuse.com\/index.php\/wp-json\/wp\/v2\/tags?post=618869"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}