{"id":784963,"date":"2024-06-28T15:45:17","date_gmt":"2024-06-28T20:45:17","guid":{"rendered":"http:\/\/spaceweekly.com\/?p=784963"},"modified":"2024-06-28T15:45:17","modified_gmt":"2024-06-28T20:45:17","slug":"volcanic-plumes-rise-above-lava-lakes-on-io-in-this-juno-image","status":"publish","type":"post","link":"https:\/\/spaceweekly.com\/?p=784963","title":{"rendered":"Volcanic Plumes Rise Above Lava Lakes on Io in this Juno Image"},"content":{"rendered":"<p> <br \/>\n<\/p>\n<div>\n<p>As the most volcanic object in the Solar System, Jupiter\u2019s moon Io attracts a lot of attention. NASA\u2019s Juno spacecraft arrived at the Jovian system in July 2016, and in recent months, it\u2019s been paying closer attention to Io.<\/p>\n<p>Though Io\u2019s internal workings have been mostly inscrutable, images and data from Juno are starting to provide a fuller picture of the strange moon\u2019s volcanic inner life. <\/p>\n<p><span id=\"more-167587\"\/><\/p>\n<p>Io\u2019s extreme volcanic activity stems from tidal heating caused by massive Jupiter and its powerful gravity. Some of the moon\u2019s volcanoes spew out plumes of sulphur and sulphur dioxide as high as 500 km (300 miles) above its surface. Sulphur is also ever-present in its lava flows, which colour the moon\u2019s surface in various shades of yellow, red, white, green, and black. Some of the lava flows extend up to 500 km (300 miles) along its surface. These features entice scientists to study the moon more thoroughly. <\/p>\n<p>One of Juno\u2019s instruments is an imager and spectrometer that operates in the infrared. It\u2019s called JIRAM (Jovian Infrared Auroral Mapper.) It was designed to, obviously, map Jupiter\u2019s aurorae. But as Juno\u2019s orbits have brought it progressively closer to Io, JIRAM is delivering high-quality images and data from the volcanic moon. <\/p>\n<figure class=\"wp-block-pullquote\">\n<blockquote>\n<p>\u201cThe observations show fascinating new information on Io\u2019s volcanic processes.\u201d<\/p>\n<p><cite>Scott Bolton, Principal Investigator for Juno, SwRI<\/cite><\/p><\/blockquote>\n<\/figure>\n<p>In new research in Nature Communications Earth and Environment, a team of scientists present some new insights into the moon and its vigorous volcanic activity. The title is \u201cHot rings on Io observed by Juno\/JIRAM.\u201d The lead author is Alessandro Mura from the National Institute of Astrophysics\u2014Institute of Space Astrophysics and Planetology, Rome, Italy. Italy provided the JIRAM instrument for the Juno mission. <\/p>\n<p>\u201cWe are just starting to wade into the JIRAM results from the close flybys of Io in December 2023 and February 2024,\u201d said Scott Bolton, principal investigator for Juno at the Southwest Research Institute in San Antonio. \u201cThe observations show fascinating new information on Io\u2019s volcanic processes. Combining these new results with Juno\u2019s longer-term campaign to monitor and map the volcanoes on Io\u2019s never-before-seen north and south poles, JIRAM is turning out to be one of the most valuable tools to learn how this tortured world works.\u201d<\/p>\n<p>Io has many of what planetary scientists call \u2018paterae.\u2019 Paterae are irregular craters or complex craters with scalloped edges. They\u2019re usually broad and shallow, and scientists have wondered if they hold lava lakes. Older observations of Io from NASA\u2019s Galileo spacecraft were inconclusive, but new images from Juno and JIRAM have much higher resolution. <\/p>\n<figure class=\"wp-block-embed is-type-video is-provider-youtube wp-block-embed-youtube wp-embed-aspect-16-9 wp-has-aspect-ratio\">\n<p>\n<span class=\"embed-youtube\" style=\"text-align:center; display: block;\"><iframe loading=\"lazy\" title=\"Looking Into Io\u2019s Loki Patera (Artist\u2019s Concept)\" width=\"1110\" height=\"624\" src=\"https:\/\/www.youtube.com\/embed\/lg2Szj_OG_Q?feature=oembed\" frameborder=\"0\" allow=\"accelerometer; autoplay; clipboard-write; encrypted-media; gyroscope; picture-in-picture; web-share\" referrerpolicy=\"strict-origin-when-cross-origin\" allowfullscreen><\/iframe><\/span>\n<\/p>\n<\/figure>\n<p>In 2023, Juno came to within 13,000 km (8,100 miles) of Io\u2019s surface, allowing JIRAM to capture greater detail. These images show more detail for a greater number of paterae, and the features the images reveal suggest that many of the craters have active lava lakes. \u201cThis new Juno\/JIRAM data suggests that hot rings around paterae are a common phenomenon, and that they are indicative of active lava lakes,\u201d the authors write in their paper. <\/p>\n<figure class=\"wp-block-image size-large\"><figcaption class=\"wp-element-caption\">This graphic shows the infrared radiance of Chors Patera, a lava lake on Jupiter\u2019s moon Io. The white ring is the hottest part of the patera, between 232 and 732 Celsius, where lava from the moon\u2019s interior is exposed. The red\/green inside the ring is likely a thick crust of molten material that\u2019s -43 Celsius. Outside the patera, the temperature is about -143 Celsius. Image Credit: NASA\/JPL-Caltech\/SwRI\/ASI\/INAF\/JIRAM\/MSSS<\/figcaption><\/figure>\n<p>\u201cThe high spatial resolution of JIRAM\u2019s infrared images, combined with the favorable position of Juno during the flybys, revealed that the whole surface of Io is covered by lava lakes contained in caldera-like features,\u201d said Alessandro Mura, the paper\u2019s lead author. \u201cIn the region of Io\u2019s surface in which we have the most complete data, we estimate about 3% of it is covered by one of these molten lava lakes.\u201d<\/p>\n<p>Outstanding questions remain about the nature of Io\u2019s volcanic activity and what happens underground. These new images help provide answers. <\/p>\n<p>The lava lakes have only a thin ring of exposed lava. There are no lava flows beyond the rim or inside the rim, which indicates a balance between the magma that erupted into the lake and the magma that flowed back underground. <\/p>\n<figure class=\"wp-block-image size-large\"><img loading=\"lazy\" decoding=\"async\" width=\"1024\" height=\"749\" src=\"https:\/\/www.universetoday.com\/wp-content\/uploads\/2024\/06\/Six-Io-Paterae-infrared-rings-1024x749.jpg\" alt=\"This figure from the research shows infrared radiance maps for six different paterae on Io. Each one has a lava ring inside the patera's rim. Image Credit: Mura et al. 2024. \" class=\"wp-image-167590\" srcset=\"https:\/\/www.universetoday.com\/wp-content\/uploads\/2024\/06\/Six-Io-Paterae-infrared-rings-1024x749.jpg 1024w, https:\/\/www.universetoday.com\/wp-content\/uploads\/2024\/06\/Six-Io-Paterae-infrared-rings-580x424.jpg 580w, https:\/\/www.universetoday.com\/wp-content\/uploads\/2024\/06\/Six-Io-Paterae-infrared-rings-250x183.jpg 250w, https:\/\/www.universetoday.com\/wp-content\/uploads\/2024\/06\/Six-Io-Paterae-infrared-rings-768x562.jpg 768w, https:\/\/www.universetoday.com\/wp-content\/uploads\/2024\/06\/Six-Io-Paterae-infrared-rings.jpg 1158w\" sizes=\"auto, (max-width: 767px) 89vw, (max-width: 1000px) 54vw, (max-width: 1071px) 543px, 580px\"\/><figcaption class=\"wp-element-caption\">This figure from the research shows infrared radiance maps for six different paterae on Io. Each one has a lava ring inside the patera\u2019s rim. Image Credit: Mura et al. 2024. <\/figcaption><\/figure>\n<p>\u201cWe now have an idea of what is the most frequent type of volcanism on Io: enormous lakes of lava where magma goes up and down,\u201d said Mura. \u201cThe lava crust is forced to break against the walls of the lake, forming the typical lava ring seen in Hawaiian lava lakes. The walls are likely hundreds of meters high, which explains why magma is generally not observed spilling out of the paterae and moving across the moon\u2019s surface.\u201d<\/p>\n<p>The researchers proposed two different geologic models to explain the lava lakes in Io\u2019s paterae: one they call a \u201ccentral upwelling model\u201d and the other a \u201cpiston motion\u201d model. <\/p>\n<p>The central upwelling model explains that the insulating crust \u201cspreads radially via convection processes in the lake and then sinks at the edges, exposing lava,\u201d the authors explain in their research. Basically, heat rises in the patera\u2019s center, pushes outward radially, and hot lava founders at the edge and is exposed. <\/p>\n<p>The problem with that model is the uniformity of the magma crust. JIRAM\u2019s images show uniform heat across the magma crust, meaning it would have to be the same thickness. How could it maintain the same thickness while radiating horizontally? <\/p>\n<p>The piston motion is slightly different. In that model, \u201ca simple up-and-down \u2018piston-type\u2019 movement of the entire lake surface may cause disruption of the lava lake crust against the patera walls to reveal hotter material,\u201d the authors explain. There\u2019s no radiating horizontal motion like the central upwelling; rather, the entire lake moves up and down. <\/p>\n<p>That model has problems, too. \u201cFor the piston-type lake model, the consistency between individual patera as well as the uniform brightness around the lake perimeter also poses geological challenges,\u201d the authors explain. For all of the ten patera in the study to have hot rings of exposed lava, the vertical motion must be ongoing at all sites. At some sites, JIRAM should\u2019ve detected changes in the depths of the patera. \u201cNo such depth changes at a specific patera have been reported,\u201d the authors note, while also writing that the images may lack the temporal and spatial resolution to detect depth changes. <\/p>\n<figure class=\"wp-block-image size-large\"><img loading=\"lazy\" decoding=\"async\" width=\"1024\" height=\"575\" src=\"https:\/\/www.universetoday.com\/wp-content\/uploads\/2024\/06\/Two-Io-paterae-models-1024x575.jpg\" alt=\"This figure from the research shows the two models the researchers are proposing. On the left in A and B is the central upwelling model. On the right in C and D is the piston motion model. Image Credit: Mura et al. 2024.\" class=\"wp-image-167591\" srcset=\"https:\/\/www.universetoday.com\/wp-content\/uploads\/2024\/06\/Two-Io-paterae-models-1024x575.jpg 1024w, https:\/\/www.universetoday.com\/wp-content\/uploads\/2024\/06\/Two-Io-paterae-models-580x325.jpg 580w, https:\/\/www.universetoday.com\/wp-content\/uploads\/2024\/06\/Two-Io-paterae-models-250x140.jpg 250w, https:\/\/www.universetoday.com\/wp-content\/uploads\/2024\/06\/Two-Io-paterae-models-768x431.jpg 768w, https:\/\/www.universetoday.com\/wp-content\/uploads\/2024\/06\/Two-Io-paterae-models.jpg 1397w\" sizes=\"auto, (max-width: 767px) 89vw, (max-width: 1000px) 54vw, (max-width: 1071px) 543px, 580px\"\/><figcaption class=\"wp-element-caption\">This figure from the research shows the two models the researchers are proposing. On the left in A and B is the central upwelling model. On the right in C and D is the piston motion model. Image Credit: Mura et al. 2024.<\/figcaption><\/figure>\n<p>Activity at the rim where the lava is hottest may hold the eventual answer. \u201cThe observation of activity at the borders of the lake raises the question of whether some type of thermal or mechanical erosion between the lake surface and the patera walls might be taking place,\u201d the authors write. Paterae might grow larger over time, but only by as much as a few hundred meters each year. No changes have been noted between visits by Voyager, Galileo, and Juno. It\u2019s still possible, but the data is inconclusive. <\/p>\n<p>The Juno spacecraft may still be able to provide deeper answers to Io\u2019s volcanic activity. It\u2019s already completed closer flybys of Io, and that data will be available in the future. <\/p>\n<p>\u201cOnce the last Juno data are acquired, examining visible images of inactive patera for signs of former lava lake activity would be instructive,\u201d the authors write in their conclusion. <\/p>\n<div class=\"sharedaddy sd-block sd-like jetpack-likes-widget-wrapper jetpack-likes-widget-unloaded\" id=\"like-post-wrapper-24000880-167587-667f1e631d9f8\" data-src=\"https:\/\/widgets.wp.com\/likes\/?ver=13.2#blog_id=24000880&amp;post_id=167587&amp;origin=www.universetoday.com&amp;obj_id=24000880-167587-667f1e631d9f8&amp;n=1\" data-name=\"like-post-frame-24000880-167587-667f1e631d9f8\" data-title=\"Like or Reblog\">\n<h3 class=\"sd-title\">Like this:<\/h3>\n<p><span class=\"button\"><span>Like<\/span><\/span> <span class=\"loading\">Loading&#8230;<\/span><\/p>\n<p><span class=\"sd-text-color\"\/><\/div>\n<\/p><\/div>\n<p><br \/>\n<br \/><a href=\"https:\/\/www.universetoday.com\/167587\/volcanic-plumes-rise-above-lava-lakes-on-io-in-this-juno-image\/?rand=772204\">Source link <\/a><\/p>\n","protected":false},"excerpt":{"rendered":"<p>As the most volcanic object in the Solar System, Jupiter\u2019s moon Io attracts a lot of attention. NASA\u2019s Juno spacecraft arrived at the Jovian system in July 2016, and in&hellip; <\/p>\n","protected":false},"author":1,"featured_media":784964,"comment_status":"closed","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[13],"tags":[],"class_list":["post-784963","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-genaero"],"_links":{"self":[{"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/posts\/784963","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=784963"}],"version-history":[{"count":0,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/posts\/784963\/revisions"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/media\/784964"}],"wp:attachment":[{"href":"https:\/\/spaceweekly.com\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=784963"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=784963"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=784963"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}