{"id":24960,"date":"2021-06-18T20:05:08","date_gmt":"2021-06-18T12:05:08","guid":{"rendered":"https:\/\/wp-productionenv-bjg9h2g2bgg5b8aa.southeastasia-01.azurewebsites.net\/news\/europa-volcanism-interior-heating-modeled-in-detail-offers-research-targets-for-upcoming-missions\/"},"modified":"2021-06-18T20:05:08","modified_gmt":"2021-06-18T12:05:08","slug":"europa-volcanism-interior-heating-modeled-in-detail-offers-research-targets-for-upcoming-missions","status":"publish","type":"post","link":"https:\/\/starpath.global\/news\/europa-volcanism-interior-heating-modeled-in-detail-offers-research-targets-for-upcoming-missions\/","title":{"rendered":"Europa volcanism &#038; interior heating modeled in detail, offers research targets for upcoming missions"},"content":{"rendered":"<p>Europa, an icy Jovian moon that likely possesses an ocean beneath its icy crust, may have an interior that is hot enough to produce volcanic activity on its seafloor. New research provides evidence that this seafloor volcanism likely occurred in the moon\u2019s past and maybe ongoing at present as well.<\/p>\n<p>The team of researchers, led by Dr. Marie B\u011bhounkov\u00e1 of Charles University in the Czech Republic, developed their own 3D models of Europa\u2019s interior and heating transfer properties to investigate the possibility of volcanism on Europa\u2019s ocean floor given other volcanism seen in the Jovian system.<\/p>\n<\/p>\n<p>Scientists have proposed the idea of a subsurface ocean under Europa\u2019s crust for years, and have strong evidence from multiple missions to support the theory. B\u011bhounkov\u00e1 et al.\u2019s new research provides evidence to the idea that that seafloor could be volcanically active.<\/p>\n<p>These volcanoes would form due to the melting of Europa\u2019s interior and heat transfer from the rocky interior of Europa to the seafloor. Models developed by Be\u030chounkov\u00e1 et al. show that many different factors \u2014 including radiogenic power and tidal forces \u2014 contribute to the melting of the icy moon\u2019s interior.<\/p>\n<p>But why this type of research regarding Europa?<\/p>\n<p>\u201cIn the Jovian system, it is known that there is huge activity on the moon Io, so we wanted to explore if it\u2019s a possibility that there is something similar, although, to a lesser extent, going on on Europa,\u201d said Dr. B\u011bhounkov\u00e1 in an interview with NASASpaceflight.<\/p>\n<p>The paper, \u201cTidally Induced Magmatic Pulses on the Oceanic Floor of Jupiter\u2019s Moon Europa\u201d was published in the journal&nbsp;<em>Geophysical Research Letters&nbsp;<\/em>the can be found here.<\/p>\n<p>Aerospace &amp; Defense<path d=\"M7.59009 18.59L9.00009 20L17.0001 12L9.00009 4L7.59009 5.41L14.1701 12\" style=\"animation: initial !important; background: initial !important; border: 0px !important; box-shadow: none !important; color: inherit !important; cursor: inherit !important; direction: inherit !important; display: inline !important; fill: currentcolor !important; filter: initial !important; float: none !important; margin: 0px !important; opacity: initial !important; outline: 0px !important; overflow: initial !important; padding: 0px !important; stroke: initial !important; transform: initial !important; vertical-align: initial !important; visibility: inherit !important;\"><\/path>Rocket building kits<path d=\"M7.59009 18.59L9.00009 20L17.0001 12L9.00009 4L7.59009 5.41L14.1701 12\" style=\"animation: initial !important; background: initial !important; border: 0px !important; box-shadow: none !important; color: inherit !important; cursor: inherit !important; direction: inherit !important; display: inline !important; fill: currentcolor !important; filter: initial !important; float: none !important; margin: 0px !important; opacity: initial !important; outline: 0px !important; overflow: initial !important; padding: 0px !important; stroke: initial !important; transform: initial !important; vertical-align: initial !important; visibility: inherit !important;\"><\/path>Astronomy<path d=\"M7.59009 18.59L9.00009 20L17.0001 12L9.00009 4L7.59009 5.41L14.1701 12\" style=\"animation: initial !important; background: initial !important; border: 0px !important; box-shadow: none !important; color: inherit !important; cursor: inherit !important; direction: inherit !important; display: inline !important; fill: currentcolor !important; filter: initial !important; float: none !important; margin: 0px !important; opacity: initial !important; outline: 0px !important; overflow: initial !important; padding: 0px !important; stroke: initial !important; transform: initial !important; vertical-align: initial !important; visibility: inherit !important;\"><\/path>\n<p>     (adsbygoogle = window.adsbygoogle || []).push({});<\/p>\n<p>However, the extent of volcanism depends on how much melting is occurring and how heat is transferred to the seafloor.<\/p>\n<\/p>\n<p><iframe title=\"Europa: Ocean World\" src=\"https:\/\/www.youtube.com\/embed\/kz9VhCQbPAk?feature=oembed\" frameborder=\"0\" allow=\"accelerometer; autoplay; clipboard-write; encrypted-media; gyroscope; picture-in-picture; web-share\" allowfullscreen=\"\" name=\"fitvid0\" data-gtm-yt-inspected-14=\"true\" data-gtm-yt-inspected-21=\"true\"><\/iframe><\/p>\n<p>B\u011bhounkov\u00e1 et al. modeled Europa\u2019s internal heating to understand exactly where and how this melting and volcanic activity is occurring. Their model is the most detailed of Europa\u2019s interior ever developed and represents the internal heat production and transfer throughout the moon\u2019s history.<\/p>\n<p>A prime candidate for the mechanism behind Europa\u2019s heating is tidal forces imparted to it via gravitational interactions with Jupiter, Io, and Ganymede. And those forces can be difficult to model.<\/p>\n<p>\u201cFrom a point of view of numerical modeling for moons and planets, tidal heating is more difficult to model because of the interaction with other bodies. This is something many people are working on now, not only in the Jovian system, but also for extrasolar planets.\u201d<\/p>\n<p>In the case of creating the model for Europa, the team had to consider the moon\u2019s changing orbital parameters over the course of its 4.5+ billion year existence. \u201cThe evolution of orbital parameters is, in our case, only parameterized. But in this case, the main influence on this evolution is Io, which we didn\u2019t model in our case. So that\u2019s why we studied several parametric models for the eccentricity evolution.\u201d<\/p>\n<p>This is in part due to the Laplace resonance of Europa with Io and Ganymede. A Laplace resonance is a phenomenon that occurs when three planetary bodies with an orbital period ratio of 1:2:4 exert regular and periodic gravitational effects on each other. These nudges create tidal forces that translate to the heating of the body\u2019s interior.<\/p>\n<p>It\u2019s that interaction that led B\u011bhounkov\u00e1 et al.\u2019s research toward the conclusion that this resonance and the associate tidal forces can cause increased periods of volcanic activity \u2014 called magmatic pulses \u2014 on Europa.<\/p>\n<p>\u201cThese magmatic pulses are basically periods of increased volcanic activity which can be induced by changes in orbital parameters \u2014 in this case, [the moon\u2019s changing] eccentricity [and its] Laplace resonance with Io and Ganymede.\u201d<\/p>\n<p><iframe id=\"twitter-widget-1\" scrolling=\"no\" frameborder=\"0\" allowtransparency=\"true\" allowfullscreen=\"true\" class=\"\" style=\"position: static; visibility: visible; width: 250px; height: 497px; display: block; flex-grow: 1;\" title=\"X Post\" src=\"https:\/\/platform.twitter.com\/embed\/Tweet.html?creatorScreenName=haygenwarren&amp;dnt=true&amp;embedId=twitter-widget-1&amp;features=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%3D%3D&amp;frame=false&amp;hideCard=false&amp;hideThread=false&amp;id=1397648234596732929&amp;lang=en&amp;origin=https%3A%2F%2Fwww.nasaspaceflight.com%2F2021%2F06%2Feuropa-heating-volcamism-study%2F&amp;sessionId=c8d07caf97746b5370790c900754c0cb003d0cbc&amp;siteScreenName=NASASpaceflight&amp;theme=light&amp;widgetsVersion=6a3ad42b224df%3A1778106238597&amp;width=550px\" data-gtm-yt-inspected-14=\"true\" data-gtm-yt-inspected-21=\"true\" data-tweet-id=\"1397648234596732929\"><\/iframe><\/p>\n<p>These magmatic pulses on Europa would result in the release of volatiles from silicate melt locations on the seafloor. \u201cThat silicate melting can produce this volcanism on the top of the mantle or the bottom of the ocean,\u201d said Dr. B\u011bhounkov\u00e1.<\/p>\n<p>Additionally, the model developed by Dr. B\u011bhounkov\u00e1 and her team shows that Europa\u2019s eccentricity evolution is periodic, which suggests increased periods of magmatic pulses on the moon.<\/p>\n<p>\u201cThere are models that the eccentricity evolution can be periodic, with increased periods of eccentricity which would induce a higher volcanic activity. The volcanic activity can be important as a source of energy for the chemical environment on the floor of Europa\u2019s ocean.\u201d<\/p>\n<p>However, tidal forces created by the Laplace resonance and Europa\u2019s changing eccentricity has not always been the leading cause of internal melting. For the first few billion years of the moon\u2019s formation, radiogenic power would have been the main cause of mantle melting and volcanism on the Jovian moon.<\/p>\n<p>However, due to radiogenic decay, this source of heating ends up having less control over Europa\u2019s internal melting rate over the course of the moon\u2019s evolution, allowing orbital eccentricity and the Laplace resonance effects to take over as the more dominate mechanisms.<\/p>\n<p>\u201cOn the other hand, the tidal evolution can be slightly different, and tidal flexing can also evolve with time. And based on eccentricity and interaction with other bodies, it can even increase with time. This is the principal difference between the radiogenic sources of energy and tidal sources of energy.\u201d<\/p>\n<p>Tidal heating is the reason why Io is so volcanically active, and as Dr. B\u011bhounkov\u00e1 said, Io\u2019s tidally heated volcanism is one of the reasons why her team wanted to research Europa for the same phenomena.<\/p>\n<p><img fetchpriority=\"high\" decoding=\"async\" aria-describedby=\"caption-attachment-78509\" class=\"size-full wp-image-78509\" src=\"https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2021\/06\/Europa-interior.jpg\" alt=\"\" width=\"700\" height=\"665\" srcset=\"https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2021\/06\/Europa-interior.jpg 700w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2021\/06\/Europa-interior-350x333.jpg 350w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2021\/06\/Europa-interior-368x350.jpg 368w\" sizes=\"(max-width: 700px) 100vw, 700px\"><\/p>\n<p id=\"caption-attachment-78509\" class=\"wp-caption-text\">Europa may consist of an iron core, surrounded by a rocky mantle in direct contact with an ocean under the icy crust. New research models how internal heat may fuel volcanoes on the seafloor. (Credit: NASA\/JPL-Caltech\/Michael Carroll)<\/p>\n<p>Based on the model created by B\u011bhounkov\u00e1 et al., Europa\u2019s heating from tidal forces is not uniformly distributed around its oceanic surface. High latitude regions near the poles are much more prone to tidal heating melting of rock and associated volcanism than at the equatorial regions, where cold downwellings typically prohibit enhanced amounts of melting to occur.<\/p>\n<p>Despite the difficulties with modeling, B\u011bhounkov\u00e1 et al.\u2019s research shows that Europa was likely very active \u2014 from a volcanism standpoint \u2014 during its years of development and is likely still an active world today.&nbsp;<\/p>\n<p>So what does this all mean, and why is this model of Europa\u2019s heating environment and volcanic history (and present) so important?<\/p>\n<p>It comes down to the moon\u2019s ocean. Where there is water and heat energy on Earth, there is life \u2014 even in the deepest recesses of the planet\u2019s oceans, where hydrothermal vents support thriving colonies of various lifeforms.<\/p>\n<p>As B\u011bhounkov\u00e1 et al. state in their paper, \u201cThe occurrence of magmatic activity on the seafloor is essential to determine if it constitutes an environment hospitable to life.\u201d &nbsp;<\/p>\n<p>They continue, stating, \u201cJupiter\u2019s icy moon Europa harbors underneath tectonically modified ice shell (Figueredo &amp; Greeley, 2004; Kattenhorn &amp; Prockter, 2014) a salty ocean (Kivelson et al., 2000) in direct contact with a rocky interior that may still be active (Moore &amp; Hussmann, 2009). Such an oceanic environment makes Europa a primary target in the search for a habitable world beyond Earth (Hand et al. 2009).\u201d<\/p>\n<p>\u201cThe chemical evolution of Europa\u2019s ocean and its habitability is conditioned by the interaction with the rocky seafloor (Vance et al., 2016). It depends on the heat released from the deep interior to the seafloor (Altair et al., 2018), and hence by the intensity of magmatic activity.\u201d<\/p>\n<p>But one sticking point remains: how to prove the model is correct and how to prove that volcanism did occur and is still occurring today?<\/p>\n<p><iframe id=\"twitter-widget-2\" scrolling=\"no\" frameborder=\"0\" allowtransparency=\"true\" allowfullscreen=\"true\" class=\"\" style=\"position: static; visibility: visible; width: 250px; height: 381px; display: block; flex-grow: 1;\" title=\"X Post\" src=\"https:\/\/platform.twitter.com\/embed\/Tweet.html?creatorScreenName=haygenwarren&amp;dnt=true&amp;embedId=twitter-widget-2&amp;features=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%3D%3D&amp;frame=false&amp;hideCard=false&amp;hideThread=false&amp;id=1296455037577764866&amp;lang=en&amp;origin=https%3A%2F%2Fwww.nasaspaceflight.com%2F2021%2F06%2Feuropa-heating-volcamism-study%2F&amp;sessionId=c8d07caf97746b5370790c900754c0cb003d0cbc&amp;siteScreenName=NASASpaceflight&amp;theme=light&amp;widgetsVersion=6a3ad42b224df%3A1778106238597&amp;width=550px\" data-gtm-yt-inspected-14=\"true\" data-gtm-yt-inspected-21=\"true\" data-tweet-id=\"1296455037577764866\"><\/iframe><\/p>\n<p>For decades, Europa has been one of the select few locations in our solar system where life is proposed to have possibly existed or exist currently. Because of this, dozens of missions have been proposed to visit the moon.<\/p>\n<p>Two upcoming flights, NASA\u2019s Europa Clipper and ESA\u2019s JUpiter ICy moons Explorer (JUICE), will specifically study Europa.<\/p>\n<p>While these spacecraft do not feature the proper instruments needed to perform a detailed study of seafloor volcanism on the Jovian moons, they can still be incredibly helpful in unlocking Europa\u2019s heating and volcanism history.<\/p>\n<p>\u201cThere will still be many things we can work with,\u201d said Dr. B\u011bhounkov\u00e1. \u201cThere will be better constraints on the evolution of orbital parameters which can help to determine the condition inside the bodies. There will be gravimeters, and the gravity field will be known with better accuracy than we know right now.\u201d<\/p>\n<p>\u201cThis can also help, and this can possibly detect some large anomalies on the seafloor. If we are lucky, we can detect some chemical and water species. It will be interesting for us to have this data and, basically, narrow the possibilities, of what\u2019s going on in Europa and Jovian system.\u201d<\/p>\n<p>JUICE is currently targeting launch on a Ariane 5 rocket no earlier than 9 June 2022. After five gravity assist maneuvers with Earth, Venus, and Mars, the craft will enter Jupiter\u2019s orbit in October 2029 before dispatching a dedicated orbiter to Ganymede for a September 2032 orbital arrival around that moon.<\/p>\n<p>Europa Clipper meanwhile is currently scheduled to launch no earlier than 10 October 2024 on a U.S. commercial launch vehicle \u2014 which almost certainly will be SpaceX\u2019s Falcon Heavy due to numerous NASA studies on which commercial vehicles were viable alternatives to the US Congress\u2019s original law that shackled the craft to the SLS rocket.<\/p>\n<p>If launched in 2024 on a Falcon Heavy, Europa Clipper will perform two gravity assists with Mars and Earth in February 2025 and December 2026, respectively, before entering orbit of Jupiter on 11 April 2030.<\/p>\n<p><i>(Lead image: Europa Credit: NASA\/JPL-Caltech\/SETI Institute)<\/i><\/p>\n","protected":false},"excerpt":{"rendered":"<p>Europa, an icy Jovian moon that likely possesses an ocean beneath its icy crust, may have an interior that is hot enough to produce volcanic activity on its seafloor. New research provides evidence that this seafloor volcanism likely occurred in the moon\u2019s past and maybe ongoing at present as well. The team of researchers, led [&hellip;]<\/p>\n","protected":false},"author":1,"featured_media":0,"comment_status":"","ping_status":"","sticky":false,"template":"","format":"standard","meta":{"_acf_changed":false,"inline_featured_image":false,"footnotes":"","_links_to":"","_links_to_target":""},"categories":[2],"tags":[1659,1282,1605,1606,8126],"class_list":["post-24960","post","type-post","status-publish","format-standard","hentry","category-news","tag-europa","tag-europa-clipper","tag-juice","tag-jupiter","tag-volcanism"],"acf":[],"_links":{"self":[{"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/posts\/24960"}],"collection":[{"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/comments?post=24960"}],"version-history":[{"count":0,"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/posts\/24960\/revisions"}],"wp:attachment":[{"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/media?parent=24960"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/categories?post=24960"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/tags?post=24960"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}