{"id":8296,"date":"2022-02-22T09:14:35","date_gmt":"2022-02-22T14:14:35","guid":{"rendered":"https:\/\/spaceandplanetarynewswire.com\/?p=8296"},"modified":"2022-02-22T09:14:35","modified_gmt":"2022-02-22T14:14:35","slug":"a-hot-jupiters-dark-side-is-revealed-in-detail-for-first-time","status":"publish","type":"post","link":"https:\/\/spaceandplanetarynewswire.com\/?p=8296","title":{"rendered":"A \u201cHot Jupiter\u2019s\u201d Dark Side Is Revealed in Detail for First Time"},"content":{"rendered":"
Caption:An artists\u2019s impression of WASP-121 b. Credits:Credit: Mikal Evans<\/figcaption><\/figure>\n

MIT astronomers have obtained the clearest view yet of the perpetual dark side of an exoplanet that is \u201ctidally locked\u201d to its star. Their observations, combined with measurements of the planet\u2019s permanent day side, provide the first detailed view of an exoplanet\u2019s global atmosphere.<\/p>\n

\u201cWe\u2019re now moving beyond taking isolated snapshots of specific regions of exoplanet atmospheres, to study them as the 3D systems they truly are,\u201d says Thomas Mikal-Evans, who led the study as a postdoc in MIT\u2019s Kavli Institute for Astrophysics and Space Research.<\/p>\n

The planet at the center of the new study<\/a>, which appears in Nature Astronomy<\/em>, is WASP-121b, a massive gas giant nearly twice the size of Jupiter. The planet is an ultrahot Jupiter and was discovered in 2015 orbiting a star about 850 light years from Earth. WASP-121b has one of the shortest orbits detected to date, circling its star in just 30 hours. It is also tidally locked, such that its star-facing \u201cday\u201d side is permanently roasting, while its \u201cnight\u201d side is turned forever toward space.  <\/p>\n

\u201cHot Jupiters are famous for having very bright day sides, but the night side is a different beast. WASP-121b’s night side is about 10 times fainter than its day side,\u201d says Tansu Daylan, a TESS postdoc at MIT who co-authored the study.<\/p>\n

Astronomers had previously detected water vapor and studied how the atmospheric temperature changes with altitude on the planet\u2019s day side.<\/p>\n

The new study captures a much more detailed picture. The researchers were able to map the dramatic temperature changes from the day to the night side, and to see how these temperatures change with altitude. They also tracked the presence of water through the atmosphere to show, for the first time, how water circulates between a planet\u2019s day and night sides.<\/p>\n

While on Earth, water cycles by first evaporating, then condensing into clouds, then raining out, on WASP-121b, the water cycle is far more intense: On the day side, the atoms that make up water are ripped apart at temperatures over 3,000 Kelvin. These atoms are blown around to the night side, where colder temperatures allow hydrogen and oxygen atoms to recombine into water molecules, which then blow back to the day side, where the cycle starts again.<\/p>\n

The team calculates that the planet\u2019s water cycle is sustained by winds that whip the atoms around the planet at speeds of up to 5 kilometers per second, or more than 11,000 miles per hour.<\/p>\n

It also appears that water isn\u2019t alone in circulating around the planet. The astronomers found that the night side is cold enough to host exotic clouds of iron and corundum \u2014 a mineral that makes up rubies and sapphires. These clouds, like water vapor, may whip around to the day side, where high temperatures vaporize the metals into gas form. On the way, exotic rain might be produced, such as liquid gems from the corundum clouds.<\/p>\n

\u201cWith this observation, we\u2019re really getting a global view of an exoplanet\u2019s meteorology,\u201d Mikal-Evans says.<\/p>\n

The study\u2019s co-authors include collaborators from MIT, Johns Hopkins University, Caltech, and other institutions.  <\/p>\n

Day and night<\/strong><\/p>\n

The team observed WASP-121b using a spectroscopic camera aboard NASA\u2019s Hubble Space Telescope. The instrument observes the light from a planet and its star, and breaks that light down into its constituent wavelengths, the intensities of which give astronomers clues to an atmosphere\u2019s temperature and composition.<\/p>\n

Through spectroscopic studies, scientists have observed atmospheric details on the day sides of many exoplanets. But doing the same for the night side is far trickier, as it requires watching for tiny changes in the planet\u2019s entire spectrum as it circles its star.<\/p>\n

For the new study, the team observed WASP-121b throughout two full orbits \u2014 one in 2018, and the other in 2019. For both observations, the researchers looked through the light data for a specific line, or spectral feature, that indicated the presence of water vapor.<\/p>\n

\u201cWe saw this water feature and mapped how it changed at different parts of the planet\u2019s orbit,\u201d Mikal-Evans says. \u201cThat encodes information about what the temperature of the planet\u2019s atmosphere is doing as a function of altitude.\u201d<\/p>\n

The changing water feature helped the team map the temperature profile of both the day and night side. They found the day side ranges from 2,500 Kelvin at its deepest observable layer, to 3,500 Kelvin in its topmost layers. The night side ranged from 1,800 Kelvin at its deepest layer, to 1,500 Kelvin in its upper atmosphere. Interestingly, temperature profiles appeared to flip-flop, rising with altitude on the day side\u2014 a \u201cthermal inversion,\u201d in meteorological terms \u2014 and dropping with altitude on the night side.<\/p>\n

The researchers then passed the temperature maps through various models to identify chemicals that are likely to exist in the planet\u2019s atmosphere, given specific altitudes and temperatures. This modeling revealed the potential for metal clouds, such as iron, corundum, and titanium on the night side.<\/p>\n

From their temperature mapping, the team also observed that the planet\u2019s hottest region is shifted to the east of the \u201csubstellar\u201d region directly below the star. They deduced that this shift is due to extreme winds.<\/p>\n

\u201cThe gas gets heated up at the substellar point but is getting blown eastward before it can reradiate to space,\u201d Mikal-Evans explains.<\/p>\n

From the size of the shift, the team estimates that the wind speeds clock in at around 5 kilometers per second.<\/p>\n

\u201cThese winds are much faster than our jet stream, and can probably move clouds across the entire planet in about 20 hours,\u201d says Daylan, who led previous work on the planet using NASA\u2019s MIT-led mission, TESS.<\/p>\n

The astronomers have reserved time on the James Webb Space Telescope to observe WASP-121b later this year, and hope to map changes in not just water vapor but also carbon monoxide, which scientists suspect should reside in the atmosphere.<\/p>\n

\u201cThat would be the first time we could measure a carbon-bearing molecule in this planet\u2019s atmosphere,\u201d Mikal-Evans says. \u201cThe amount of carbon and oxygen in the atmosphere provides clues on where these kinds of planet form.\u201d<\/p>\n","protected":false},"excerpt":{"rendered":"

MIT astronomers have obtained the clearest view yet of the perpetual dark side of an exoplanet that is \u201ctidally locked\u201d to its star. Their observations, combined with measurements of the planet\u2019s permanent day side, provide the first detailed view of an exoplanet\u2019s global atmosphere. \u201cWe\u2019re now moving beyond taking isolated snapshots of specific regions of…<\/p>\n","protected":false},"author":71,"featured_media":8298,"comment_status":"open","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"ngg_post_thumbnail":0,"fifu_image_url":"https:\/\/news.mit.edu\/sites\/default\/files\/images\/202202\/MIT_Jupiter-Night-01-PRESS.jpg","fifu_image_alt":"A \u201cHot Jupiter\u2019s\u201d Dark Side Is Revealed in Detail for First Time","footnotes":""},"categories":[216],"tags":[],"class_list":["post-8296","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-discovery"],"_links":{"self":[{"href":"https:\/\/spaceandplanetarynewswire.com\/index.php?rest_route=\/wp\/v2\/posts\/8296","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=8296"}],"version-history":[{"count":1,"href":"https:\/\/spaceandplanetarynewswire.com\/index.php?rest_route=\/wp\/v2\/posts\/8296\/revisions"}],"predecessor-version":[{"id":8297,"href":"https:\/\/spaceandplanetarynewswire.com\/index.php?rest_route=\/wp\/v2\/posts\/8296\/revisions\/8297"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/spaceandplanetarynewswire.com\/index.php?rest_route=\/wp\/v2\/media\/8298"}],"wp:attachment":[{"href":"https:\/\/spaceandplanetarynewswire.com\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=8296"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/spaceandplanetarynewswire.com\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=8296"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/spaceandplanetarynewswire.com\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=8296"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}