{"id":43414,"date":"2023-04-18T06:45:31","date_gmt":"2023-04-18T06:45:31","guid":{"rendered":"https:\/\/blogs.agu.org\/landslideblog\/?p=43414"},"modified":"2023-04-18T06:45:31","modified_gmt":"2023-04-18T06:45:31","slug":"icy-satellites-1","status":"publish","type":"post","link":"https:\/\/blogs.agu.org\/landslideblog\/2023\/04\/18\/icy-satellites-1\/","title":{"rendered":"Landslides as a dominant landscape process on icy satellites"},"content":{"rendered":"<h4><strong>Landslides as a dominant landscape process on icy satellites<\/strong><\/h4>\n<p>The journal <a href=\"https:\/\/www.sciencedirect.com\/journal\/icarus\"><em>Icarus<\/em><\/a> has a very interesting new paper (<a href=\"https:\/\/www.sciencedirect.com\/science\/article\/pii\/S0019103523001112\">Mills <em>et al.<\/em> 2023<\/a>) that considers why some icy satellites of large planets, such as those orbiting Jupiter and Saturn (in particular Ganymede, Europa, and Enceladus), have smooth surfaces with very few impact craters.\u00a0 There is a good plain English summary of this work on the <a href=\"https:\/\/interestingengineering.com\/science\/nasa-icy-moons-jupiter-saturn\">Interesting Engineering website<\/a> too.\u00a0 Conventionally, the theory has been that the smooth surfaces have been created by the eruption of fluids from volcanoes.<\/p>\n<div id=\"attachment_43417\" style=\"width: 590px\" class=\"wp-caption alignnone\"><img loading=\"lazy\" decoding=\"async\" aria-describedby=\"caption-attachment-43417\" class=\"size-full wp-image-43417\" src=\"https:\/\/blogs.agu.org\/landslideblog\/files\/2023\/04\/23_04-Ganymede-1.jpg\" alt=\"The topography of Ganymede, an icy satellite of Jupiter. \" width=\"580\" height=\"491\" srcset=\"https:\/\/blogs.agu.org\/landslideblog\/files\/2023\/04\/23_04-Ganymede-1.jpg 580w, https:\/\/blogs.agu.org\/landslideblog\/files\/2023\/04\/23_04-Ganymede-1-300x254.jpg 300w\" sizes=\"auto, (max-width: 580px) 100vw, 580px\" \/><p id=\"caption-attachment-43417\" class=\"wp-caption-text\"><em>The topography of Ganymede, an icy satellite of Jupiter. <a href=\"https:\/\/phys.org\/news\/2015-10-jupiter-moon-ganymede.html\">Image NASA via phys.org<\/a><\/em><\/p><\/div>\n<p>.<\/p>\n<p>Interestingly, these icy satellites are known to be geologically-active, resulting from the high gravitational forces from the planets, which generate planetary seismic events (the equivalent of terrestrial earthquakes).\u00a0 This geological activity has created ridges, with smooth surfaces between them.\u00a0 The authors test the hypothesis that the seismic events trigger landslides from these ridges, which then mantle the surface of the icy satellite to create the smooth topography.<\/p>\n<p><a href=\"https:\/\/www.sciencedirect.com\/science\/article\/pii\/S0019103523001112\">Mills <em>et al.<\/em> (2023<\/a>) have used the dimensions of the fault scarps to estimate the magnitude of the seismic events (the ranger is M=4.0 to 7.9), and then have modelled the resulting seismic accelerations.\u00a0 These accelerations were found to be sufficiently large to exceed the gravitational accelerations of the satellites, allowing mass movements to develop.\u00a0 The team has assessed the potential volumes of the resultant landslides, using two different models.\u00a0 The more recent of these suggests that for Ganymede for example, the landslide volumes could be in the range of 2.3 \u00d7 10<sup>6<\/sup>\u20131.4\u00a0\u00d7\u00a010<sup>9<\/sup>\u00a0 cubic metres.\u00a0 It must be stressed that these are quite speculative &#8211; there are many assumptions implicit in that number &#8211; but it is a very interesting result.<\/p>\n<p>There is much work to do on this idea, which will be greatly assisted by the forthcoming <a href=\"https:\/\/astronomy.com\/news\/2023\/04\/two-missions-target-jupiters-moons\">Europa Clipper and JUICE missions<\/a>, which are intended to &#8220;provide high-resolution surface imaging, including stereo imaging, along with subsurface radar sounding, for both Europa and Ganymede&#8221;.<\/p>\n<p>This study is another illustration of the key role that landslides play in planetary systems.<\/p>\n<p>.<\/p>\n<h5>Reference<\/h5>\n<p>Mills, M.M.,\u00a0 Pappalardo, R.T., Panning, M.P. et al. 2023.\u00a0 <a href=\"https:\/\/www.sciencedirect.com\/science\/article\/pii\/S0019103523001112\">Moonquake-triggered mass wasting processes on icy satellites<\/a>.\u00a0 <em>Icarus<\/em>, <strong>399<\/strong>, 115534.\u00a0 <a href=\"https:\/\/doi.org\/10.1016\/j.icarus.2023.115534\">https:\/\/doi.org\/10.1016\/j.icarus.2023.115534<\/a>.<\/p>\n<p>&nbsp;<\/p>\n<!-- AddThis Advanced Settings generic via filter on the_content --><!-- AddThis Share Buttons generic via filter on the_content -->","protected":false},"excerpt":{"rendered":"<p>Landslides as a dominant landscape process on icy satellites The journal Icarus has a very interesting new paper (Mills et al. 2023) that considers why some icy satellites of large planets, such as those orbiting Jupiter and Saturn (in particular Ganymede, Europa, and Enceladus), have smooth surfaces with very few impact craters.\u00a0 There is a good plain English summary of this work on the Interesting Engineering website too.\u00a0 Conventionally, the &hellip;<!-- AddThis Advanced Settings generic via filter on wp_trim_excerpt --><!-- AddThis Share Buttons generic via filter on wp_trim_excerpt --><\/p>\n","protected":false},"author":22,"featured_media":43417,"comment_status":"open","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[1],"tags":[469,30743,15447,17,788],"class_list":["post-43414","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-uncategorized","tag-featured","tag-jupiter","tag-planetary-landslide","tag-research","tag-review-of-a-paper-2"],"_links":{"self":[{"href":"https:\/\/blogs.agu.org\/landslideblog\/wp-json\/wp\/v2\/posts\/43414","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/blogs.agu.org\/landslideblog\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/blogs.agu.org\/landslideblog\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/blogs.agu.org\/landslideblog\/wp-json\/wp\/v2\/users\/22"}],"replies":[{"embeddable":true,"href":"https:\/\/blogs.agu.org\/landslideblog\/wp-json\/wp\/v2\/comments?post=43414"}],"version-history":[{"count":0,"href":"https:\/\/blogs.agu.org\/landslideblog\/wp-json\/wp\/v2\/posts\/43414\/revisions"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/blogs.agu.org\/landslideblog\/wp-json\/wp\/v2\/media\/43417"}],"wp:attachment":[{"href":"https:\/\/blogs.agu.org\/landslideblog\/wp-json\/wp\/v2\/media?parent=43414"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/blogs.agu.org\/landslideblog\/wp-json\/wp\/v2\/categories?post=43414"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/blogs.agu.org\/landslideblog\/wp-json\/wp\/v2\/tags?post=43414"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}