{"id":10097,"date":"2020-01-02T09:30:00","date_gmt":"2020-01-02T14:30:00","guid":{"rendered":"http:\/\/all-geo.org\/highlyallochthonous\/?p=10097"},"modified":"2020-01-02T09:31:57","modified_gmt":"2020-01-02T14:31:57","slug":"can-we-detect-plate-tectonics-on-exoplanets","status":"publish","type":"post","link":"https:\/\/all-geo.org\/highlyallochthonous\/2020\/01\/can-we-detect-plate-tectonics-on-exoplanets\/","title":{"rendered":"Can we detect plate tectonics on exoplanets?"},"content":{"rendered":"\n<p>As celebrated in this&nbsp;<a href=\"https:\/\/arstechnica.com\/science\/2019\/12\/the-2010s-decade-of-the-exoplanet\/\">Ars Technica piece<\/a>, the 2010s was &#8216;the decade of the exoplanet&#8217;. Largely thanks to the Kepler telescope, the past ten years has seen an explosion in exoplanet discoveries.&nbsp;<a href=\"http:\/\/exoplanet.eu\/catalog\/\">More than 4000 planets<\/a>&nbsp;have now been identified orbiting other stars, generally arranged in ways not at all like our own solar system.&nbsp;<\/p>\n\n\n\n<p>It\u2019s very exciting, particular for a space junkie like me*, who grew up reading space books that discussed the possibility of the solar system being totally unique in the Universe. I have a hard time nowadays believing astronomers seriously thought this, but the point is that we had no evidence either way.<\/p>\n\n\n\n<p>Nowadays, geologist me greedily wonders if we can look for signatures of active geology. And it turns out that maybe you can.&nbsp;<a href=\"https:\/\/www.liebertpub.com\/doi\/10.1089\/ast.2014.1204\">This paper<\/a>&nbsp;(see also the&nbsp;<a href=\"https:\/\/exoplanets.nasa.gov\/news\/196\/seeking-life-on-other-worlds-check-for-volcanoes\/\">write-up here<\/a>, and there is a&nbsp;<a href=\"https:\/\/arxiv.org\/pdf\/1504.04629.pdf\">version on arXiv<\/a>&nbsp;if you have problems accessing the version of record) suggests if an exoplanet&#8217;s atmosphere is monitored, we could potentially detect the spike of sulphate aerosols injected into the stratosphere by large explosive eruptions (such as the 1991 Pinatubo eruption).<\/p>\n\n\n\n<p>You might be wondering how we can know anything about the composition of an exoplanetary atmosphere, let alone detect a change. It depends on a technique known  as &#8216;<a href=\"https:\/\/www.physics.uu.se\/research\/astronomy-and-space-physics\/research\/planets\/exoplanet-atmospheres\/\">transit spectroscopy<\/a>&#8216;. When it passes in front of its star, gases in an exoplanet&#8217;s atmosphere (if it has one) will absorb some of the star&#8217;s light. Different gases absorb light at different frequencies, so we can get data on the composition of what is doing the blocking.   <\/p>\n\n\n\n<p>Detecting a volcanic eruption across light years would be a pretty amazing feat in itself, but on Earth the most common cause of large explosive eruptions is silica and gas-rich magmas generated at subduction zones &#8211; so this particular kind of volcanic signature is at least potentially a signal of plate-tectonic like recycling of the lithosphere specifically, and not just volcanism generally.<\/p>\n\n\n\n<p>Unfortunately, the sensitivity required to detect a sulphate aerosol spike is beyond the capabilities of current telescopes. But good news! Imminently operational telescopes such as the&nbsp;<a href=\"https:\/\/www.jwst.nasa.gov\/\">James Webb Space Telescope<\/a>&nbsp;(allegedly) and the&nbsp;<a href=\"https:\/\/www.eso.org\/sci\/facilities\/eelt\/\">Extremely Large Telescope<\/a>&nbsp;<em>would<\/em>&nbsp;potentially be able to make such a detection. However, there is a small caveat: even these new telescopes will only be able to reliably make a detection on Earth-sized planets within about 30 light years of Earth. The authors estimate that there are likely to be less than 10 of those, which is not a great sample size. On the one hand, if we don&#8217;t detect anything, it doesn&#8217;t really tell us much definitive. On the other hand, if we <em>do<\/em> find an explosively volcanic planet on one of our first tries, it might indicate that geologically active Earth-ish planets, that turn themselves inside out, are relatively common.&nbsp;<\/p>\n\n\n\n<p>This would be&nbsp;<em>very<\/em>&nbsp;cool. Let&#8217;s hope that the next generation of telescopes gets lucky.<\/p>\n\n\n\n<p>*If there are parallel universes, there is almost certainly a fairly adjacent one where I pursued my original science career goal of astronomy and astrophysics; if so, I\u2019m pretty sure that alt-Chris is all about the (exo)planets.<\/p>\n","protected":false},"excerpt":{"rendered":"<p>As celebrated in this&nbsp;Ars Technica piece, the 2010s was &#8216;the decade of the exoplanet&#8217;. Largely thanks to the Kepler telescope, the past ten years has seen an explosion in exoplanet discoveries.&nbsp;More than 4000 planets&nbsp;have now been identified orbiting other stars, &hellip; <a href=\"https:\/\/all-geo.org\/highlyallochthonous\/2020\/01\/can-we-detect-plate-tectonics-on-exoplanets\/\">Continue reading <span class=\"meta-nav\">&rarr;<\/span><\/a><\/p>\n","protected":false},"author":2,"featured_media":0,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[4,15,19,12],"tags":[308,850,85],"class_list":["post-10097","post","type-post","status-publish","format-standard","hentry","category-geology","category-planets","category-tectonics","category-volcanoes","tag-exoplanets","tag-kepler","tag-plate-tectonics"],"_links":{"self":[{"href":"https:\/\/all-geo.org\/highlyallochthonous\/wp-json\/wp\/v2\/posts\/10097","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/all-geo.org\/highlyallochthonous\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/all-geo.org\/highlyallochthonous\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/all-geo.org\/highlyallochthonous\/wp-json\/wp\/v2\/users\/2"}],"replies":[{"embeddable":true,"href":"https:\/\/all-geo.org\/highlyallochthonous\/wp-json\/wp\/v2\/comments?post=10097"}],"version-history":[{"count":3,"href":"https:\/\/all-geo.org\/highlyallochthonous\/wp-json\/wp\/v2\/posts\/10097\/revisions"}],"predecessor-version":[{"id":10100,"href":"https:\/\/all-geo.org\/highlyallochthonous\/wp-json\/wp\/v2\/posts\/10097\/revisions\/10100"}],"wp:attachment":[{"href":"https:\/\/all-geo.org\/highlyallochthonous\/wp-json\/wp\/v2\/media?parent=10097"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/all-geo.org\/highlyallochthonous\/wp-json\/wp\/v2\/categories?post=10097"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/all-geo.org\/highlyallochthonous\/wp-json\/wp\/v2\/tags?post=10097"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}