{"id":774729,"date":"2023-11-29T18:28:51","date_gmt":"2023-11-29T23:28:51","guid":{"rendered":"http:\/\/spaceweekly.com\/?p=774729"},"modified":"2023-11-29T18:28:51","modified_gmt":"2023-11-29T23:28:51","slug":"it-doesnt-take-much-to-get-tilted-planets","status":"publish","type":"post","link":"https:\/\/spaceweekly.com\/?p=774729","title":{"rendered":"It Doesn&#8217;t Take Much to Get Tilted Planets"},"content":{"rendered":"<p> <br \/>\n<\/p>\n<div>\n<p>Chinese and Indian astronomers were the first to measure Earth\u2019s axial tilt accurately, and they did it about 3,000 years ago. Their measurements were remarkably accurate: in 1120 BC, Chinese astronomers pegged the Earth\u2019s axial tilt at 24 degrees. Now we know that all of the planets in the Solar System, with the exception of Mercury, have some tilt. <\/p>\n<p>While astronomers have puzzled over why our Solar System\u2019s planets are tilted, it turns out it\u2019s rather normal.<\/p>\n<p><span id=\"more-164520\"\/><\/p>\n<p>Now that astronomers have observed so many other solar systems, they\u2019ve learned that axial tilt is to be expected, even in so-called \u201cpristine\u201d solar systems. Pristine refers to the precise mathematical relationship between planets. <\/p>\n<p>New research in The Astronomical Journal explains why some axial tilt is to be expected. It\u2019s titled \u201cEvidence for Low-level Dynamical Excitation in Near-resonant Exoplanet Systems.\u201d The lead author is Malena Rice, an assistant professor of astronomy at Yale\u2019s Faculty of Arts and Sciences.<\/p>\n<p>The orbital resonance concept is at the heart of this research. <\/p>\n<p>As planets orbit a star, they can exert regular and periodic gravitational influence on one another. When they do, astronomers say they\u2019re in resonance with one another. It also happens in moon systems around planets with many moons. Some resonant systems can be self-stabilizing, while others can become unstabilized over time. <\/p>\n<figure class=\"wp-block-embed is-type-video is-provider-youtube wp-block-embed-youtube wp-embed-aspect-4-3 wp-has-aspect-ratio\">\n<p>\n<span class=\"embed-youtube\" style=\"text-align:center; display: block;\"><iframe loading=\"lazy\" title=\"Orbital Resonance of Jupiter&#039;s Moons - As a Beat\" width=\"1110\" height=\"833\" src=\"https:\/\/www.youtube.com\/embed\/L3h_OIHU5pc?feature=oembed\" frameborder=\"0\" allow=\"accelerometer; autoplay; clipboard-write; encrypted-media; gyroscope; picture-in-picture; web-share\" allowfullscreen><\/iframe><\/span>\n<\/p><figcaption class=\"wp-element-caption\">This video does a good job of illustrating orbital resonance using three of Jupiter\u2019s moons. <\/figcaption><\/figure>\n<p>Early in a solar system\u2019s history, planets are more likely to be in resonance with one another. <\/p>\n<p>\u201cThis type of configuration, where one planet\u2019s orbit is precisely ordered with another in an exact integer ratio of orbital periods, is likely common to find in a solar system early in its development,\u201d said Rice. \u201cIt\u2019s a gorgeous configuration \u2014 but only a small percentage of systems retain it.\u201d <\/p>\n<p>\u201cGiven that near-resonant systems have likely experienced minimal dynamical disruptions, the spin-orbit orientations of these systems inform the typical outcomes of quiescent planet formation, as well as the primordial stellar obliquity distribution,\u201d the authors write in their research. The spin-orbit orientation is the tilt of companion planets\u2019 orbits relative to the host star\u2019s spin axis.<\/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=\"Planets and dwarf planets to scale in size, rotation speed &amp; axial tilt in distance order from Sun\" width=\"1110\" height=\"624\" src=\"https:\/\/www.youtube.com\/embed\/hf6WUmwJKZE?feature=oembed\" frameborder=\"0\" allow=\"accelerometer; autoplay; clipboard-write; encrypted-media; gyroscope; picture-in-picture; web-share\" allowfullscreen><\/iframe><\/span>\n<\/p>\n<\/figure>\n<p>What that boils down to is that in a system that\u2019s suffered few disruptions, like migrating planets, for example, the spin-orbit and axial tilt of the planets in the system should be largely unchanged from the time of formation. But the problem is astronomers haven\u2019t rigorously measured the spin-orbit orientations of near-resonant systems. <\/p>\n<p>\u201cTo date, only a handful of near-resonant systems have had spin-orbit angles measured to characterize the tilts of their constituent planetary orbits,\u201d the authors explain in their research. <\/p>\n<p>In this work, the researchers started out by examining a warm Jupiter named TOI-2202 b. It\u2019s a near-resonant planet that\u2019s only slightly less massive than Jupiter. It orbits a K-type star about 770 light-years away. TOI-2202 b is tight to its star, only 0.09564 AU away, and it completes an orbit in only 11.9 days. For comparison, Mercury is 0.387098 AU away from the Sun. <\/p>\n<p>TOI-2202 b is in a pristine solar system, and it\u2019s in a 2:1 mean-motion resonance with another planet further from the star. The researchers compared it to archival data and new observations of the exoplanet from multiple telescopes. They arrived at a spin-orbit angle of about 31 degrees. Then they compared that to the full census of other similar planets in pristine systems found in NASA\u2019s Exoplanet Archive. <\/p>\n<p>\u201cTo place this measurement into context, we examined the full set of transiting exoplanet systems with (1) a sky-projected spin-orbit measurement and (2) evidence that the transiting planet lies near a low-order mean-motion resonance with a neighbouring companion,\u201d the authors explain in their research.<\/p>\n<p>They found that planets in these pristine systems exhibit a typical spin-orbit angle of around 20 degrees. So even \u201cquiet\u201d solar systems have axial tilt. TOI-2202 b was one of the most strongly tilted planets in the sample. \u201cThe measured spin-orbit angle of TOI-2202 b, together with the full census of spin-orbit measurements for near-resonant exoplanets, indicates that even quiescently formed systems may experience low-level dynamical excitation that produces some dispersion in their spin-orbit orientations,\u201d the authors write.<\/p>\n<figure class=\"wp-block-image size-large\"><figcaption class=\"wp-element-caption\">This is an artist\u2019s illustration of TOI-2202 b. Image Credit: NASA<\/figcaption><\/figure>\n<p>This told the researchers that our Solar System\u2019s tilted planets are the norm rather than an oddball outlier. <\/p>\n<p>\u201cIt\u2019s reassuring,\u201d Rice said. \u201cIt tells us that we\u2019re not a super-weird solar system. This is really like looking at ourselves in a funhouse mirror and seeing how we fit into the bigger picture of the universe.\u201d<\/p>\n<p>Our Solar System does contain one oddball, though: Uranus. Uranus\u2019s tilt angle is 97.77 degrees, nearly parallel to the Solar System\u2019s plane. Astronomers aren\u2019t certain, but a collision with an Earth-sized protoplanet in the Solar System\u2019s early days is likely the cause. <\/p>\n<p>One of Rice\u2019s research areas concerns hot Jupiters and why they exhibit such pronounced axial tilts. \u201cI\u2019m trying to figure out why systems with hot Jupiters have such extremely tilted orbits,\u201d Rice said. \u201cWhen did they get tilted? Can they just be born that way? To find that out, I first need to find out what types of systems are not so dramatically tilted.\u201d<\/p>\n<p>That search continues.<\/p>\n<div class=\"sharedaddy sd-block sd-like jetpack-likes-widget-wrapper jetpack-likes-widget-unloaded\" id=\"like-post-wrapper-24000880-164520-6567c89480e96\" data-src=\"https:\/\/widgets.wp.com\/likes\/#blog_id=24000880&amp;post_id=164520&amp;origin=www.universetoday.com&amp;obj_id=24000880-164520-6567c89480e96\" data-name=\"like-post-frame-24000880-164520-6567c89480e96\" 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\/164520\/it-doesnt-take-much-to-get-tilted-planets\/?rand=772204\">Source link <\/a><\/p>\n","protected":false},"excerpt":{"rendered":"<p>Chinese and Indian astronomers were the first to measure Earth\u2019s axial tilt accurately, and they did it about 3,000 years ago. Their measurements were remarkably accurate: in 1120 BC, Chinese&hellip; <\/p>\n","protected":false},"author":1,"featured_media":774730,"comment_status":"closed","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[13],"tags":[],"class_list":["post-774729","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\/774729","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=774729"}],"version-history":[{"count":0,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/posts\/774729\/revisions"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/media\/774730"}],"wp:attachment":[{"href":"https:\/\/spaceweekly.com\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=774729"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=774729"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=774729"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}