{"id":793569,"date":"2025-02-13T11:29:05","date_gmt":"2025-02-13T16:29:05","guid":{"rendered":"https:\/\/spaceweekly.com\/?p=793569"},"modified":"2025-02-13T11:29:05","modified_gmt":"2025-02-13T16:29:05","slug":"a-balloon-with-a-tether-could-explore-venus-surface","status":"publish","type":"post","link":"https:\/\/spaceweekly.com\/?p=793569","title":{"rendered":"A Balloon With a Tether Could Explore Venus&#8217; Surface"},"content":{"rendered":"<p> <br \/>\n<\/p>\n<div>\n<p>Venus is very variable. Its surface constantly changes from volcanic activity, and the difference between its lower and upper atmosphere is night and day, with a dramatic change in sulfuric acid concentration. So, designing a system that works for all parts of Venus is particularly challenging. NASA thinks they might be on to a new idea of how to do so and has funded Ben Hockman, a roboticist at the Jet Propulsion Laboratory, to work on a tethered atmospheric sensor attached to a balloon as part of the NASA Institute of Advanced Concepts Phase I program.<\/p>\n<p><span id=\"more-170888\"\/><\/p>\n<p>The project, known as the Tethered Observatory for Balloon-based Imaging and Atmospheric Sampling (TOBIAS\u2014assumedly not after the Arrested Development character), is based on a simple principle. On Venus, a very distinct cloud layer, between 47 and 52 km in altitude, separates the relatively stable upper atmosphere similar to Earth\u2019s, with a hellish surface that no probes have yet lasted longer than a few minutes on.\u00a0<\/p>\n<p>TOBIAS would float a helium-filled balloon in the upper atmosphere, where conditions are Earth-like. Then it would release a \u201ctowbody\u201d \u2013 a stand-alone sensing platform connected to the balloon by a tether. That tether is intended to be several kilometers long, allowing the towbody to pass through the hazardous cloud layer and, hopefully, take accurate, high-resolution images of Venus\u2019 surface.<\/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<iframe loading=\"lazy\" title=\"Our Best Venus Map Is 36 Years Old. NASA Wants to Fix it With Balloons [NIAC 2025]\" width=\"1110\" height=\"624\" src=\"https:\/\/www.youtube.com\/embed\/BePPHPj6uo8?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>\n<\/p><figcaption class=\"wp-element-caption\">Fraser interviews Ben Hockman, the PI for the TOBIAS project.<\/figcaption><\/figure>\n<p>Several design decisions will be the focus of the Phase I NIAC grant. According to Dr. Hockman\u2019s interview with Fraser, one of the most important aspects will be the tether design. The most significant force on the tether wouldn\u2019t be from the towbody itself but from the wind shear. The wind conditions are different enough from where the balloon is located (50-60km altitude) to where the towbody is intended to reside (45km altitude) that the forces on the tether would be strong enough to rip it apart if it\u2019s not designed correctly.<\/p>\n<p>Also, the tether\u2019s material is essential. Standard copper wire could potentially power the towbody, but it would be too heavy to survive the mission\u2019s expected wind shear conditions. Optical fiber could prove a viable alternative, but there are some concerns about the amount of power that could be transmitted that way. According to Dr. Hockman, \u201cPeople have put power over fiber before.\u201d<\/p>\n<p>Much of that power would go to a cooling system that would make the temperature in that part of the Venusian atmosphere manageable. Dr. Hockman suggests alternative power sources, like solar panels (which would be affected by the same cloud layer that obscures the surface) to wind turbines, which would do well because of the high energy available from the wind but might lead to stability issues with the towbody.<\/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<iframe loading=\"lazy\" title=\"Here&#039;s Why We Need A Venus Exploration Program\" width=\"1110\" height=\"624\" src=\"https:\/\/www.youtube.com\/embed\/qshaDSStFPY?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>\n<\/p><figcaption class=\"wp-element-caption\">Fraser explains why Venus is a critical step in our space exploration program.<\/figcaption><\/figure>\n<p>Ultimately, if they can get the cable, power, and communication systems on the towbody to work, it could provide atmospheric sensing, and more importantly, direct imaging of the surface of Venus, in a variety of wavelengths. Near-infrared images, which TOBIAS could supply, could help answer outstanding questions about the history of Venusian volcanism.<\/p>\n<p>Dr. Hockman even speculates about the potential for a tethered impactor to land on the surface, grab a sample, and reel itself back up to the balloon. That concept was the subject of a previous year\u2019s NIAC grant, though it\u2019s unclear whether further progress has been made.<\/p>\n<p>TOBIAS would benefit from additional information about the Venusian atmosphere from DaVinci and Veritas, which will also contain instruments to peer through to the surface, just not in the wavelengths that the towbody would enable. Data from those missions could inform the design of TOBIAS\u2019s balloon and tether system, hopefully making it more likely to survive Venus\u2019 extreme conditions.<\/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<iframe loading=\"lazy\" title=\"Developing Tech That Can Last On Venus\" width=\"1110\" height=\"624\" src=\"https:\/\/www.youtube.com\/embed\/iVtquFgZ2pQ?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>\n<\/p><figcaption class=\"wp-element-caption\">Venus presents a ton of engineering challenges, as Fraser discusses here.<\/figcaption><\/figure>\n<p>The project still has a long way to go before it has to survive anything, though. NIAC grants, especially Phase I, are meant to encourage very early design studies, many of which are unlikely to receive further funding. But, if Dr. Hockman proves the idea more and receives a Phase II grant sometime in the next few years, a balloon tugging along some sensors might one day reach Venusian skies.<\/p>\n<p>Learn More:<br \/>NASA \/ Ben Hockman \u2013 TOBIAS: Tethered Observatory for Balloon-based Imaging and Atmospheric Sampling<br \/>UT \u2013 A Balloon Mission That Could Explore Venus Indefinitely<br \/>UT \u2013 The Best Way to Learn About Venus Could Be With a Fleet of Balloons<br \/>UT \u2013 Is There Seismic Activity on Venus? Here\u2019s How We Could Find Out<\/p>\n<p>Lead Image:<br \/>Artist\u2019s concept of TOBIAS<br \/>Credit \u2013 Ben Hockman \/ NASA<\/p>\n<div class=\"sharedaddy sd-block sd-like jetpack-likes-widget-wrapper jetpack-likes-widget-unloaded\" id=\"like-post-wrapper-24000880-170888-67ae1bf8b3d40\" data-src=\"https:\/\/widgets.wp.com\/likes\/?ver=14.0#blog_id=24000880&amp;post_id=170888&amp;origin=www.universetoday.com&amp;obj_id=24000880-170888-67ae1bf8b3d40&amp;n=1\" data-name=\"like-post-frame-24000880-170888-67ae1bf8b3d40\" 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\/170888\/a-balloon-with-a-tether-could-explore-venus-surface\/?rand=772204\">Source link <\/a><\/p>\n","protected":false},"excerpt":{"rendered":"<p>Venus is very variable. Its surface constantly changes from volcanic activity, and the difference between its lower and upper atmosphere is night and day, with a dramatic change in sulfuric&hellip; <\/p>\n","protected":false},"author":1,"featured_media":793570,"comment_status":"closed","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[13],"tags":[],"class_list":["post-793569","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\/793569","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=793569"}],"version-history":[{"count":0,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/posts\/793569\/revisions"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/media\/793570"}],"wp:attachment":[{"href":"https:\/\/spaceweekly.com\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=793569"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=793569"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=793569"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}