{"id":8683,"date":"2022-12-09T03:49:55","date_gmt":"2022-12-09T08:49:55","guid":{"rendered":"https:\/\/spaceandplanetarynewswire.com\/?p=8683"},"modified":"2022-12-09T03:49:55","modified_gmt":"2022-12-09T08:49:55","slug":"how-the-hell-planet-got-so-hot","status":"publish","type":"post","link":"https:\/\/spaceandplanetarynewswire.com\/?p=8683","title":{"rendered":"How the \u2018Hell Planet\u2019 Got So Hot"},"content":{"rendered":"<figure style=\"width: 700px\" class=\"wp-caption alignnone\"><img decoding=\"async\" class=\"size-medium\" src=\"https:\/\/earimediaprodweb.azurewebsites.net\/Api\/v1\/Multimedia\/00fb310e-21d8-4e69-9e03-73bab2ff7e57\/Rendition\/low-res\/Content\/Public\" width=\"700\" height=\"476\"><figcaption class=\"wp-caption-text\">An artist\u2019s impression of the planet Janssen, which orbits its star so closely that its entire surface is a lava ocean that reaches temperatures of around 2,000 degrees Celsius.<\/figcaption><\/figure>\n<p>New research sheds light on how the \u201chell planet\u201d got so devilishly hot and how other worlds might become too toasty for life. That rocky world, 55 Cnc e (nicknamed \u201cJanssen\u201d), orbits its star so closely that a year lasts just 18 hours, its surface is a giant lava ocean, and its interior may be chock-full of diamond.<\/p>\n<p>The fresh insights come thanks to a new tool called EXPRES that captured ultra-precise measurements of the starlight shining from Janssen\u2019s sun, known as Copernicus or 55 Cnc. The light measurements ever-so-slightly shifted as Janssen moved between Earth and the star (an effect akin to our moon blocking the sun during a solar eclipse).<\/p>\n<p>By analyzing those measurements, astronomers discovered that Janssen orbits Copernicus along the star\u2019s equator \u2014 unlike Copernicus\u2019 other planets, which are on such different orbital paths that they never even cross between the star and Earth,&nbsp;<a href=\"https:\/\/www.nature.com\/articles\/s41550-022-01837-2\">the researchers report December 8 in&nbsp;<em>Nature Astronomy<\/em><\/a>.<\/p>\n<p>The implication is that Janssen probably formed in a relatively cooler orbit further out and slowly fell toward Copernicus over time. As Janssen moved closer in, the stronger gravitational pull from Copernicus altered the planet\u2019s orbit.<\/p>\n<p>\u201cWe\u2019ve learned about how this multi-planet system \u2014 one of the systems with the most planets that we\u2019ve found \u2014 got into its current state,\u201d says study lead author Lily Zhao, a research fellow at the&nbsp;<a href=\"https:\/\/www.simonsfoundation.org\/flatiron\/\">Flatiron Institute<\/a>\u2019s&nbsp;<a href=\"https:\/\/www.simonsfoundation.org\/flatiron\/center-for-computational-astrophysics\/\">Center for Computational Astrophysics<\/a>&nbsp;(CCA) in New York City.<\/p>\n<figure style=\"width: 700px\" class=\"wp-caption alignnone\"><img decoding=\"async\" class=\"size-medium\" src=\"https:\/\/earimediaprodweb.azurewebsites.net\/Api\/v1\/Multimedia\/85235664-ce94-4346-b1bf-fec6e9a91609\/Rendition\/low-res\/Content\/Public\" width=\"700\" height=\"700\"><figcaption class=\"wp-caption-text\">An artist\u2019s impression of the planet Janssen (orange circle), which orbits its star so closely that its entire surface is a lava ocean that reaches temperatures of around 2,000 degrees Celsius.<\/figcaption><\/figure>\n<p>Even in its original orbit, the planet \u201cwas likely so hot that nothing we\u2019re aware of would be able to survive on the surface,\u201d Zhao says. Still, the new findings could help scientists better understand how planets form and move around over time. Such information is critical to finding out just how common Earth-like environments are in the universe and, therefore, how abundant extraterrestrial life may be.<\/p>\n<div class=\"flex-video widescreen youtube\"><iframe title=\"How the &#039;hell planet&#039; got so hot\" width=\"500\" height=\"281\" data-src=\"https:\/\/www.youtube.com\/embed\/PzblrrXR2mg?feature=oembed&#038;showinfo=0&#038;rel=0&#038;modestbranding=1&#038;iv_load_policy=3&#038;playsinline=1&#038;enablejsapi=1\" frameborder=\"0\" allow=\"accelerometer; autoplay; clipboard-write; encrypted-media; gyroscope; picture-in-picture; web-share\" referrerpolicy=\"strict-origin-when-cross-origin\" allowfullscreen src=\"data:image\/svg+xml;base64,PHN2ZyB3aWR0aD0iMSIgaGVpZ2h0PSIxIiB4bWxucz0iaHR0cDovL3d3dy53My5vcmcvMjAwMC9zdmciPjwvc3ZnPg==\" class=\"lazyload\" data-load-mode=\"0\"><\/iframe><\/div>\n<p>Our solar system, after all, is the only place in the cosmos where we know life exists. It\u2019s also flat as a pancake \u2014 all the planets orbit within a few degrees of one another, having formed from the same disk of gas and dust. When exoplanet-hunting missions started discovering worlds around distant stars, they found many planets that didn\u2019t orbit their host stars on a flat plane. This raised the question of whether our pancakelike solar system is truly a rarity.<\/p>\n<p>Copernicus\u2019 planetary system, which is 40 light-years away from Earth, is of particular interest given how well studied and complex it is: Five exoplanets orbit a main-sequence star (the most common category of star) in a binary pair with a red dwarf star. In fact, Janssen was the first \u2018super-Earth\u2019 discovered around a main-sequence star. While Janssen has a similar density to Earth and is likely rocky, it\u2019s about eight times as massive and twice as wide.<\/p>\n<p>Upon its discovery and confirmation, Janssen became the first known example of an ultra-short-period planet. Janssen\u2019s orbit has a minimum radius of roughly 2 million kilometers. (For comparison, Mercury\u2019s is 46 million kilometers, and Earth\u2019s is around 147 million.) Janssen\u2019s orbit is so snug around Copernicus that at first some astronomers doubted its existence.<\/p>\n<p>Determining Janssen\u2019s path around Copernicus could reveal much about the planet\u2019s history, but making such measurements is incredibly hard. Astronomers have studied Janssen by measuring the dip in Copernicus\u2019 brightness every time the planet comes between the star and Earth.<\/p>\n<figure style=\"width: 577px\" class=\"wp-caption alignnone\"><img decoding=\"async\" class=\"size-medium\" src=\"https:\/\/earimediaprodweb.azurewebsites.net\/Api\/v1\/Multimedia\/5f410e35-5432-4e06-b47e-a010636d62ad\/Rendition\/low-res\/Content\/Public\" width=\"577\" height=\"700\"><figcaption class=\"wp-caption-text\">A diagram of the star Copernicus (large circle) from a new study investigating how the exoplanet 55 Cnc e (nicknamed \u201cJanssen\u201d and represented by a black dot) orbits its star. The research revealed that the planet\u2019s orbit (slanted horizontal line) broadly aligns with the star\u2019s equator. This new information was obtained from precise measurements of the host star\u2019s light. As Janssen moves between the star and Earth, the measured starlight dips. The resulting change in the star\u2019s observed color depends on which half of the star Janssen is crossing. Due to the Doppler effect, the hemisphere rotating toward Earth is slightly bluer, the opposite hemisphere spinning away is somewhat redder, and the middle is unchanged.<\/figcaption><\/figure>\n<p>That method doesn\u2019t tell you what direction the planet is moving in. To find that out, astronomers take advantage of the same Doppler effect used in speeding cameras. When a light source is moving toward you, the wavelength of the light you see is shorter (and therefore bluer). When it\u2019s moving away, the frequency is shifted wider, and the light is redder.<\/p>\n<p>As Copernicus rotates, half of the star is twirling toward us, and the other half is moving away. That means half the star is a bit bluer, and the other half is slightly redder (and the space in the middle is unshifted). So astronomers can track Janssen\u2019s orbit by measuring when it\u2019s blocking light from the redder side, the bluer side and the unaltered midsection.<\/p>\n<p>The resulting difference in the starlight, however, is almost immeasurably small. Teams had tried before but couldn\u2019t accurately determine the planet\u2019s orbital path. The breakthrough in the new research came from the EXtreme PREcision Spectrometer (EXPRES) at the Lowell Observatory\u2019s Lowell Discovery Telescope in Arizona. True to its name, the spectrometer offered the precision needed to notice the light\u2019s tiny red and blue shifts.<\/p>\n<p>The EXPRES measurements revealed that Janssen\u2019s orbit is roughly aligned with Copernicus\u2019 equator, a path that makes Janssen unique among its siblings.<\/p>\n<p>Previous research suggests that the nearby orbit of the red dwarf resulted in the misalignment of the planets relative to Copernicus. In the new study, the researchers propose that interactions between the heavenly bodies shifted Janssen toward its hellish present-day location. As Janssen approached Copernicus, the star\u2019s gravity became increasingly dominant. Because Copernicus is spinning, the centrifugal force caused its midsection to bulge outward slightly and its top and bottom to flatten. That asymmetry affected the gravity felt by Janssen, pulling the planet into alignment with the star\u2019s thicker equator.<\/p>\n<p>With Janssen\u2019s history illuminated, Zhao and her colleagues now plan to study other planetary systems. \u201cWe\u2019re hoping to find planetary systems similar to ours,\u201d she says, \u201cand to better understand the systems that we do know about.\u201d<\/p>\n","protected":false},"excerpt":{"rendered":"<p>New research sheds light on how the \u201chell planet\u201d got so devilishly hot and how other worlds might become too toasty for life. That rocky world, 55 Cnc e (nicknamed \u201cJanssen\u201d), orbits its star so closely that a year lasts just 18 hours, its surface is a giant lava ocean, and its interior may be&hellip;<\/p>\n","protected":false},"author":71,"featured_media":8686,"comment_status":"open","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"ngg_post_thumbnail":0,"fifu_image_url":"https:\/\/earimediaprodweb.azurewebsites.net\/Api\/v1\/Multimedia\/00fb310e-21d8-4e69-9e03-73bab2ff7e57\/Rendition\/low-res\/Content\/Public","fifu_image_alt":"How the \u2018Hell Planet\u2019 Got So Hot","footnotes":""},"categories":[207],"tags":[],"class_list":["post-8683","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-research"],"_links":{"self":[{"href":"https:\/\/spaceandplanetarynewswire.com\/index.php?rest_route=\/wp\/v2\/posts\/8683","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/spaceandplanetarynewswire.com\/index.php?rest_route=\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/spaceandplanetarynewswire.com\/index.php?rest_route=\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/spaceandplanetarynewswire.com\/index.php?rest_route=\/wp\/v2\/users\/71"}],"replies":[{"embeddable":true,"href":"https:\/\/spaceandplanetarynewswire.com\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=8683"}],"version-history":[{"count":1,"href":"https:\/\/spaceandplanetarynewswire.com\/index.php?rest_route=\/wp\/v2\/posts\/8683\/revisions"}],"predecessor-version":[{"id":8685,"href":"https:\/\/spaceandplanetarynewswire.com\/index.php?rest_route=\/wp\/v2\/posts\/8683\/revisions\/8685"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/spaceandplanetarynewswire.com\/index.php?rest_route=\/wp\/v2\/media\/8686"}],"wp:attachment":[{"href":"https:\/\/spaceandplanetarynewswire.com\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=8683"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/spaceandplanetarynewswire.com\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=8683"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/spaceandplanetarynewswire.com\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=8683"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}