{"id":181941,"date":"2025-03-04T01:00:00","date_gmt":"2025-03-03T15:00:00","guid":{"rendered":"https:\/\/science.nasa.gov\/missions\/webb\/nasas-webb-exposes-complex-atmosphere-of-starless-super-jupiter\/"},"modified":"2025-03-04T01:00:00","modified_gmt":"2025-03-03T15:00:00","slug":"nasas-webb-exposes-complex-atmosphere-of-starless-super-jupiter","status":"publish","type":"post","link":"https:\/\/www.vibewire.com.au\/?p=181941","title":{"rendered":"NASA\u2019s Webb Exposes Complex Atmosphere of Starless Super-Jupiter"},"content":{"rendered":"<div id=\"\" class=\" hds-module hds-module-full wp-block-nasa-blocks-secondary-navigation\">\n<div class=\"hds-secondary-navigation-wrapper z-top width-100 padding-0\">\n<div id=\"\" class=\"hds-secondary-navigation width-full border-bottom-1px text-center hds-color-mode-light hds-module hds-module-full wp-block-nasa-blocks-hdsnav\"><button type=\"button\" class=\"hds-secondary-nav-mobile-button display-flex tablet:display-flex 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Fun\/Learning<\/a><\/li>\n<\/ul>\n<\/li>\n<\/ul>\n<\/nav>\n<\/div>\n<\/div>\n<\/div>\n<\/div>\n<\/div>\n<div id=\"\" class=\"hds-article-hero-header nasa-gb-align-full bg-carbon-90 width-full maxw-full color-mode-dark hds-module hds-module-full wp-block-nasa-blocks-article-hero-header\">\n<div class=\"hds-cover-wrapper width-full maxw-full minh-tablet grid-container minh-tablet flex-column padding-0\">\n<div class=\"hds-foreground-wrapper display-flex flex-direction-column\">\n<div class=\"grid-container grid-container-block margin-top-auto width-full maxw-desktop-lg padding-y-9 padding-x-3 desktop:padding-x-3 z-400\">\n<div class=\"z-400 grid-col-12 tablet:grid-col-12 desktop:grid-col-7 z-400\">\n<div class=\"margin-0\">\n<div class=\"label color-spacesuit-white margin-bottom-2\">6 Min Read<\/div>\n<h1 class=\"heading-41 line-height-md color-spacesuit-white-important\">\n\t\t\t\t\t\t\t\tNASA\u2019s Webb Exposes Complex Atmosphere of Starless Super-Jupiter\t\t\t\t\t\t\t<\/h1>\n<\/p>\n<\/div>\n<\/div>\n<div class=\"grid-col-12 tablet:grid-col-12 desktop:grid-col-5\"><\/div>\n<div class=\"skrim-overlay skrim-left mobile-skrim-top z-200\"><\/div>\n<figure class=\"hds-media-background  \"><img fetchpriority=\"high\" decoding=\"async\" width=\"1920\" height=\"1080\" src=\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2025\/webb-STScI-01JMZ7PP4XV01SZM19G2VXK1BZ-2K.jpg?w=1920&#038;h=1080&#038;%23038;fit=clip&#038;%23038;crop=faces%2Cfocalpoint\" class=\"attachment-1536x1536 size-1536x1536\" alt=\"Illustration of a large spherical object that looks like a gas giant planet or a brown dwarf. The object appears to be glowing, with wavy, horizontal bands of yellow, orange, and red forming patterns similar to those in the atmosphere of Jupiter. In the mid-latitudes of the northern hemisphere, just to the right of center, is a large, elliptical, dark red feature similar to Jupiter\u2019s Great Red Spot. Hints of a blue-green auroral glow emanate from the south pole. Larger blue-green auroral arcs descend from the north pole down toward the middle northern latitudes. The background is filled with with thousands of distant stars that form a Milky Way-like band running from left to light. The object is isolated, with no host star nearby. The words \u201cArtist\u2019s Concept\u201d are in the lower left corner of the illustration.\" style=\"transform: scale(1); transform-origin: 54% 74%; object-position: 54% 74%; object-fit: cover;\" block_context=\"nasa-block\" srcset=\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2025\/webb-STScI-01JMZ7PP4XV01SZM19G2VXK1BZ-2K.jpg?w=1920&#038;h=1080&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1920w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2025\/webb-STScI-01JMZ7PP4XV01SZM19G2VXK1BZ-2K.jpg?w=300&#038;h=169&#038;fit=crop&#038;crop=faces%2Cfocalpoint 300w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2025\/webb-STScI-01JMZ7PP4XV01SZM19G2VXK1BZ-2K.jpg?w=768&#038;h=432&#038;fit=crop&#038;crop=faces%2Cfocalpoint 768w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2025\/webb-STScI-01JMZ7PP4XV01SZM19G2VXK1BZ-2K.jpg?w=1024&#038;h=576&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1024w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2025\/webb-STScI-01JMZ7PP4XV01SZM19G2VXK1BZ-2K.jpg?w=1536&#038;h=864&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1536w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2025\/webb-STScI-01JMZ7PP4XV01SZM19G2VXK1BZ-2K.jpg?w=400&#038;h=225&#038;fit=crop&#038;crop=faces%2Cfocalpoint 400w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2025\/webb-STScI-01JMZ7PP4XV01SZM19G2VXK1BZ-2K.jpg?w=600&#038;h=338&#038;fit=crop&#038;crop=faces%2Cfocalpoint 600w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2025\/webb-STScI-01JMZ7PP4XV01SZM19G2VXK1BZ-2K.jpg?w=900&#038;h=506&#038;fit=crop&#038;crop=faces%2Cfocalpoint 900w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2025\/webb-STScI-01JMZ7PP4XV01SZM19G2VXK1BZ-2K.jpg?w=1200&#038;h=675&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1200w\" sizes=\"(max-width: 1920px) 100vw, 1920px\" loading=\"eager\" \/><\/figure>\n<\/p>\n<\/div>\n<\/div>\n<\/div>\n<div class=\"padding-y-3 padding-x-3\">\n<div class=\"grid-container grid-container-block padding-x-0\"><figcaption class=\"hds-caption maxw-mobile desktop:padding-x-3\">\n<div class=\"hds-caption-text p-sm margin-0 color-carbon-30\">\n<div><figcaption>This artist\u2019s concept shows what the isolated planetary-mass object SIMP 0136 could look like based on recent observations from NASA\u2019s James Webb Space Telescope and previous observations from Hubble, Spitzer, and numerous ground-based telescopes.<\/figcaption><\/div>\n<\/p>\n<\/div>\n<div class=\"hds-credits color-spacesuit-white-important\">\n\t\t\t\t\t\t\t<span>Credits: <\/span><br \/>\n\t\t\t\t\t\t\t<span>NASA, ESA, CSA, and Joseph Olmsted (STScI)<\/span>\n\t\t\t\t\t\t<\/div>\n<\/figcaption><\/div>\n<\/p>\n<\/div>\n<\/div>\n<p>An international team of researchers has discovered that previously observed variations in brightness of a <a href=\"https:\/\/webbtelescope.org\/glossary.html#h3-CK-33c7f384-6159-462c-ad34-23063a9b12cb\"  rel=\"noreferrer noopener\">free-floating planetary-mass object<\/a> known as SIMP 0136 must be the result of a complex combination of atmospheric factors, and cannot be explained by clouds alone.<\/p>\n<p>Using NASA\u2019s James Webb Space Telescope to monitor a broad spectrum of infrared light emitted over two full rotation periods by SIMP 0136, the team was able to detect variations in cloud layers, temperature, and carbon chemistry that were previously hidden from view.<\/p>\n<p>The results provide crucial insight into the three-dimensional complexity of gas giant atmospheres within and beyond our solar system. Detailed characterization of objects like these is essential preparation for <a href=\"https:\/\/science.nasa.gov\/mission\/roman-space-telescope\/direct-imaging\/\" rel=\"noopener\">direct imaging<\/a> of exoplanets, planets outside our solar system, with NASA\u2019s Nancy Grace Roman Space Telescope, which is scheduled to begin operations in 2027.<\/p>\n<h2 class=\"wp-block-heading\">Rapidly Rotating, Free-Floating<\/h2>\n<p>SIMP 0136 is a rapidly rotating, free-floating object roughly 13 times the mass of Jupiter, located in the Milky Way just 20 light-years from Earth. Although it is not classified as a gas giant exoplanet \u2014 it doesn\u2019t orbit a star and may instead be a <a href=\"https:\/\/webbtelescope.org\/glossary.html#h3-CK-3638b3e7-aa22-480f-83ea-d22b13081886\"  rel=\"noreferrer noopener\">brown dwarf<\/a> \u2014 SIMP 0136 is an ideal target for exo-meteorology: It is the brightest object of its kind in the northern sky. Because it is isolated, it can be observed with no fear of light contamination or variability caused by a host star. And its short rotation period of just 2.4 hours makes it possible to survey very efficiently.<\/p>\n<p>Prior to the Webb observations, SIMP 0136 had been studied extensively using ground-based observatories and NASA\u2019s Hubble and Spitzer space telescopes.<\/p>\n<p>\u201cWe already knew that it varies in brightness, and we were confident that there are patchy cloud layers that rotate in and out of view and evolve over time,\u201d explained Allison McCarthy, doctoral student at Boston University and lead author on a study published today in <a href=\"https:\/\/iopscience.iop.org\/article\/10.3847\/2041-8213\/ad9eaf\"  rel=\"noreferrer noopener\"><em>The Astrophysical Journal Letters<\/em><\/a>. \u201cWe also thought there could be temperature variations, chemical reactions, and possibly some effects of auroral activity affecting the brightness, but we weren\u2019t sure.\u201d<\/p>\n<p>To figure it out, the team needed Webb\u2019s ability to measure very precise changes in brightness over a broad range of wavelengths.<\/p>\n<h2 class=\"wp-block-heading\">Graphic A: Isolated Planetary-Mass Object SIMP 0136 (Artist\u2019s Concept)<\/h2>\n<div id=\"\" class=\"hds-media hds-module wp-block-image\">\n<div class=\"margin-left-auto margin-right-auto nasa-block-align-wide\">\n<div class=\"hds-media-wrapper margin-left-auto margin-right-auto\">\n<figure class=\"hds-media-inner hds-cover-wrapper hds-media-ratio-fit \"><a href=\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2025\/webb-STScI-01JMZ7PP4XV01SZM19G2VXK1BZ-2K.jpg?w=1920&#038;h=1080&#038;%23038;fit=clip&#038;%23038;crop=faces%2Cfocalpoint\" rel=\"noopener\"><img loading=\"lazy\" decoding=\"async\" width=\"1920\" height=\"1080\" src=\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2025\/webb-STScI-01JMZ7PP4XV01SZM19G2VXK1BZ-2K.jpg?w=1920&#038;h=1080&#038;%23038;fit=clip&#038;%23038;crop=faces%2Cfocalpoint\" class=\"attachment-2048x2048 size-2048x2048\" alt=\"Illustration of a large spherical object that looks like a gas giant planet or a brown dwarf. The object appears to be glowing, with wavy, horizontal bands of yellow, orange, and red forming patterns similar to those in the atmosphere of Jupiter. In the mid-latitudes of the northern hemisphere, just to the right of center, is a large, elliptical, dark red feature similar to Jupiter\u2019s Great Red Spot. Hints of a blue-green auroral glow emanate from the south pole. Larger blue-green auroral arcs descend from the north pole down toward the middle northern latitudes. The background is filled with with thousands of distant stars that form a Milky Way-like band running from left to light. The object is isolated, with no host star nearby. The words \u201cArtist\u2019s Concept\u201d are in the lower left corner of the illustration.\" style=\"transform: scale(1); transform-origin: 50% 50%; object-position: 50% 50%; object-fit: cover;\" block_context=\"nasa-block\" srcset=\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2025\/webb-STScI-01JMZ7PP4XV01SZM19G2VXK1BZ-2K.jpg?w=1920&#038;h=1080&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1920w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2025\/webb-STScI-01JMZ7PP4XV01SZM19G2VXK1BZ-2K.jpg?w=300&#038;h=169&#038;fit=crop&#038;crop=faces%2Cfocalpoint 300w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2025\/webb-STScI-01JMZ7PP4XV01SZM19G2VXK1BZ-2K.jpg?w=768&#038;h=432&#038;fit=crop&#038;crop=faces%2Cfocalpoint 768w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2025\/webb-STScI-01JMZ7PP4XV01SZM19G2VXK1BZ-2K.jpg?w=1024&#038;h=576&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1024w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2025\/webb-STScI-01JMZ7PP4XV01SZM19G2VXK1BZ-2K.jpg?w=1536&#038;h=864&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1536w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2025\/webb-STScI-01JMZ7PP4XV01SZM19G2VXK1BZ-2K.jpg?w=400&#038;h=225&#038;fit=crop&#038;crop=faces%2Cfocalpoint 400w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2025\/webb-STScI-01JMZ7PP4XV01SZM19G2VXK1BZ-2K.jpg?w=600&#038;h=338&#038;fit=crop&#038;crop=faces%2Cfocalpoint 600w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2025\/webb-STScI-01JMZ7PP4XV01SZM19G2VXK1BZ-2K.jpg?w=900&#038;h=506&#038;fit=crop&#038;crop=faces%2Cfocalpoint 900w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2025\/webb-STScI-01JMZ7PP4XV01SZM19G2VXK1BZ-2K.jpg?w=1200&#038;h=675&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1200w\" sizes=\"auto, (max-width: 1920px) 100vw, 1920px\" \/><\/a><\/figure><figcaption class=\"hds-caption padding-y-2\">\n<div class=\"hds-caption-text p-sm margin-0\">This artist\u2019s concept shows what the isolated planetary-mass object SIMP 0136 could look like based on recent observations from NASA\u2019s James Webb Space Telescope and previous observations from Hubble, Spitzer, and numerous ground-based telescopes. Researchers used Webb\u2019s NIRSpec (Near-Infrared Spectrograph) and MIRI (Mid-Infrared Instrument) to measure subtle changes in the brightness of infrared light as the object completed two 2.4-hour rotations. By analyzing the change in brightness of different wavelengths over time, they were able to detect variability in cloud cover at different depths, temperature variations in the upper atmosphere, and changes in carbon chemistry as different sides of the object rotated in and out of view. This illustration is based on Webb\u2019s spectroscopic observations. Webb has not captured a direct image of the object.<\/div>\n<div class=\"hds-credits\">NASA, ESA, CSA, and Joseph Olmsted (STScI)<\/div>\n<\/figcaption><\/div>\n<\/div>\n<\/div>\n<h2 class=\"wp-block-heading\">Charting Thousands of Infrared Rainbows<\/h2>\n<p>Using NIRSpec (Near-Infrared Spectrograph), Webb captured thousands of individual 0.6- to 5.3-micron spectra \u2014 one every 1.8 seconds over more than three hours as the object completed one full rotation. This was immediately followed by an observation with MIRI (Mid-Infrared Instrument), which collected hundreds of spectroscopic measurements of 5- to 14-micron light \u2014 one every 19.2 seconds, over another rotation.<\/p>\n<p>The result was hundreds of detailed light curves, each showing the change in brightness of a very precise wavelength (color) as different sides of the object rotated into view.<\/p>\n<p>\u201cTo see the full spectrum of this object change over the course of minutes was incredible,\u201d said principal investigator Johanna Vos, from Trinity College Dublin. \u201cUntil now, we only had a little slice of the near-infrared spectrum from Hubble, and a few brightness measurements from Spitzer.\u201d<\/p>\n<p>The team noticed almost immediately that there were several distinct light-curve shapes. At any given time, some wavelengths were growing brighter, while others were becoming dimmer or not changing much at all. A number of different factors must be affecting the brightness variations.<\/p>\n<p>\u201cImagine watching Earth from far away. If you were to look at each color separately, you would see different patterns that tell you something about its surface and atmosphere, even if you couldn\u2019t make out the individual features,\u201d explained co-author Philip Muirhead, also from Boston University. \u201cBlue would increase as oceans rotate into view. Changes in brown and green would tell you something about soil and vegetation.\u201d<\/p>\n<h2 class=\"wp-block-heading\">Graphic B: Isolated Planetary-Mass Object SIMP 0136 (NIRSpec Light Curves)<\/h2>\n<div id=\"\" class=\"hds-media hds-module wp-block-image\">\n<div class=\"margin-left-auto margin-right-auto nasa-block-align-wide\">\n<div class=\"hds-media-wrapper margin-left-auto margin-right-auto\">\n<figure class=\"hds-media-inner hds-cover-wrapper hds-media-ratio-fit \"><a href=\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2025\/webb-STScI-01JMZ7SPAZV1QGZSB2AFXS6DBK-2K.jpg?w=1920&#038;h=1080&#038;%23038;fit=clip&#038;%23038;crop=faces%2Cfocalpoint\" rel=\"noopener\"><img loading=\"lazy\" decoding=\"async\" width=\"1920\" height=\"1080\" src=\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2025\/webb-STScI-01JMZ7SPAZV1QGZSB2AFXS6DBK-2K.jpg?w=1920&#038;h=1080&#038;%23038;fit=clip&#038;%23038;crop=faces%2Cfocalpoint\" class=\"attachment-2048x2048 size-2048x2048\" alt=\"Infographic titled \u201cIsolated Planetary-Mass Object SIMP 0136, Change in Brightness as Object Rotates, NIRSpec Time-Series Spectroscopy\u201d with graph of Relative Brightness near-infrared emitted light on y-axis (brighter toward top) versus Time on July 23, 2023, Coordinated Universal Time (UTC) on x-axis (ranging from 7 to 10:15 PM). Three curves plotted. Red: Light from deep iron cloud layer. Yellow: Light from high silicate cloud layer. Blue: Light related to temperature high above the clouds. Curves overlap; each has different shape, with peaks and valleys of different size occurring at different times. Below curves are illustrations showing visible face of rotating object at beginning, middle, and end of 2.4-hour rotation period. To right of graph is atmosphere diagram showing red arrows coming up from deep iron cloud layer at 10 bars, yellow arrows coming from high silicate cloud layer at 1 bar, and blue arrows at top of atmosphere.\" style=\"transform: scale(1); transform-origin: 50% 50%; object-position: 50% 50%; object-fit: cover;\" block_context=\"nasa-block\" srcset=\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2025\/webb-STScI-01JMZ7SPAZV1QGZSB2AFXS6DBK-2K.jpg?w=1920&#038;h=1080&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1920w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2025\/webb-STScI-01JMZ7SPAZV1QGZSB2AFXS6DBK-2K.jpg?w=300&#038;h=169&#038;fit=crop&#038;crop=faces%2Cfocalpoint 300w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2025\/webb-STScI-01JMZ7SPAZV1QGZSB2AFXS6DBK-2K.jpg?w=768&#038;h=432&#038;fit=crop&#038;crop=faces%2Cfocalpoint 768w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2025\/webb-STScI-01JMZ7SPAZV1QGZSB2AFXS6DBK-2K.jpg?w=1024&#038;h=576&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1024w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2025\/webb-STScI-01JMZ7SPAZV1QGZSB2AFXS6DBK-2K.jpg?w=1536&#038;h=864&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1536w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2025\/webb-STScI-01JMZ7SPAZV1QGZSB2AFXS6DBK-2K.jpg?w=400&#038;h=225&#038;fit=crop&#038;crop=faces%2Cfocalpoint 400w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2025\/webb-STScI-01JMZ7SPAZV1QGZSB2AFXS6DBK-2K.jpg?w=600&#038;h=338&#038;fit=crop&#038;crop=faces%2Cfocalpoint 600w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2025\/webb-STScI-01JMZ7SPAZV1QGZSB2AFXS6DBK-2K.jpg?w=900&#038;h=506&#038;fit=crop&#038;crop=faces%2Cfocalpoint 900w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2025\/webb-STScI-01JMZ7SPAZV1QGZSB2AFXS6DBK-2K.jpg?w=1200&#038;h=675&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1200w\" sizes=\"auto, (max-width: 1920px) 100vw, 1920px\" \/><\/a><\/figure><figcaption class=\"hds-caption padding-y-2\">\n<div class=\"hds-caption-text p-sm margin-0\">These light curves show the change in brightness of three different sets of wavelengths (colors) of near-infrared light coming from the isolated planetary-mass object SIMP 0136  as it rotated. The light was captured by Webb\u2019s NIRSpec (Near-Infrared Spectrograph), which collected a total of 5,726 spectra \u2014 one every 1.8 seconds \u2014 over the course of about 3 hours on July 23, 2023. The variations in brightness are thought to be related to different atmospheric features \u2014 deep clouds composed of iron particles, higher clouds made of tiny grains of silicate minerals, and high-altitude hot and cold spots \u2014 rotating in and out of view. The diagram at the right illustrates the possible structure of SIMP 0136\u2019s atmosphere, with the colored arrows representing the same wavelengths of light shown in the light curves. Thick arrows represent more (brighter) light; thin arrows represent less (dimmer) light.<\/div>\n<div class=\"hds-credits\">NASA, ESA, CSA, and Joseph Olmsted (STScI)<\/div>\n<\/figcaption><\/div>\n<\/div>\n<\/div>\n<h2 class=\"wp-block-heading\">Patchy Clouds, Hot Spots, and Carbon Chemistry<\/h2>\n<p>To figure out what could be causing the variability on SIMP 0136, the team used atmospheric models to show where in the atmosphere each wavelength of light was originating.<\/p>\n<p>\u201cDifferent wavelengths provide information about different depths in the atmosphere,\u201d explained McCarthy. \u201cWe started to realize that the wavelengths that had the most similar light-curve shapes also probed the same depths, which reinforced this idea that they must be caused by the same mechanism.\u201d<\/p>\n<p>One group of wavelengths, for example, originates deep in the atmosphere where there could be patchy clouds made of iron particles. A second group comes from higher clouds thought to be made of tiny grains of silicate minerals. The variations in both of these light curves are related to patchiness of the cloud layers.<\/p>\n<p>A third group of wavelengths originates at very high altitude, far above the clouds, and seems to track temperature. Bright \u201chot spots\u201d could be related to auroras that were previously detected at radio wavelengths, or to upwelling of hot gas from deeper in the atmosphere.<\/p>\n<p>Some of the light curves cannot be explained by either clouds or temperature, but instead show variations related to atmospheric carbon chemistry. There could be pockets of carbon monoxide and carbon dioxide rotating in and out of view, or chemical reactions causing the atmosphere to change over time.<\/p>\n<p>\u201cWe haven\u2019t really figured out the chemistry part of the puzzle yet,\u201d said Vos. \u201cBut these results are really exciting because they are showing us that the abundances of molecules like methane and carbon dioxide could change from place to place and over time. If we are looking at an exoplanet and can get only one measurement, we need to consider that it might not be representative of the entire planet.\u201d<\/p>\n<p>This research was conducted as part of Webb\u2019s General Observer Program <a href=\"https:\/\/www.stsci.edu\/jwst-program-info\/download\/jwst\/pdf\/3548\/\"  rel=\"noreferrer noopener\">3548<\/a>.<\/p>\n<p><em>The James Webb Space Telescope is the world\u2019s premier space science observatory. Webb is solving mysteries in our solar system, looking beyond to distant worlds around other stars, and probing the mysterious structures and origins of our universe and our place in it. Webb is an international program led by NASA with its partners, ESA (European Space Agency) and CSA (Canadian Space Agency).<\/em><\/p>\n<h2 class=\"wp-block-heading\" id=\"h-downloads\">Downloads<\/h2>\n<p><strong>Right click any image to save it or open a larger version<\/strong> in a new tab\/window via the browser\u2019s popup menu.<\/p>\n<p><strong><a href=\"https:\/\/webbtelescope.org\/contents\/news-releases\/2025\/news-2025-106#section-id-2\"  rel=\"noreferrer noopener\">View\/Download all image products at all resolutions<\/a><\/strong> for this article from the Space Telescope Science Institute.<\/p>\n<p><strong>View\/Download the research results<\/strong> from <a href=\"https:\/\/iopscience.iop.org\/article\/10.3847\/2041-8213\/ad9eaf\"  rel=\"noreferrer noopener\">The Astrophysical Journal Letters<\/a>.<\/p>\n<\/p>\n<h2 class=\"wp-block-heading\" id=\"h-media-contacts\">Media Contacts<\/h2>\n<p><strong>Laura\u00a0Betz<\/strong>\u00a0\u2013\u00a0<a href=\"mailto:laura.e.betz@nasa.gov\">laura.e.betz@nasa.gov<\/a><br \/>NASA\u2019s <a href=\"http:\/\/www.nasa.gov\/goddard\"  rel=\"noreferrer noopener\">Goddard Space Flight Center<\/a>, Greenbelt, Md.<\/p>\n<p><strong>Margaret W. Carruthers<\/strong> \u2013 <a href=\"mailto:mcarruthers@stsci.edu\">mcarruthers@stsci.edu<\/a><br \/><a href=\"https:\/\/www.stsci.edu\/\"  rel=\"noreferrer noopener\">Space Telescope Science Institute<\/a>, Baltimore, Md.<\/p>\n<p><strong>Hannah Braun<\/strong> \u2013 <a href=\"mailto:hbraun@stsci.edu\">hbraun@stsci.edu<\/a><br \/><a href=\"https:\/\/www.stsci.edu\/\"  rel=\"noreferrer noopener\">Space Telescope Science Institute<\/a>, Baltimore, Md.<\/p>\n<\/p>\n<h2 class=\"wp-block-heading\" id=\"h-related-information\">Related Information<\/h2>\n<p><strong><a href=\"https:\/\/science.nasa.gov\/mission\/webb\/latestnews\/\" rel=\"noopener\">More Webb News<\/a><\/strong><\/p>\n<p><strong><a href=\"https:\/\/science.nasa.gov\/mission\/webb\/multimedia\/images\/\" rel=\"noopener\">More Webb Images<\/a><\/strong><\/p>\n<p><a href=\"https:\/\/science.nasa.gov\/mission\/webb\/science-overview\/\" rel=\"noopener\"><strong>Webb Science Themes<\/strong><\/a><\/p>\n<p><strong><a href=\"https:\/\/science.nasa.gov\/mission\/webb\/\" rel=\"noopener\">Webb Mission Page<\/a><\/strong> <\/p>\n<p><strong>Learn more about <a href=\"https:\/\/science.nasa.gov\/category\/universe\/stars\/brown-dwarfs\/\" rel=\"noopener\">brown dwarf discoveries<\/a><\/strong><\/p>\n<p><strong>Article:<\/strong> <a href=\"https:\/\/webbtelescope.org\/contents\/articles\/spectroscopy-101--types-of-spectra-and-spectroscopy\"  rel=\"noreferrer noopener\">Spectroscopy 101<\/a><\/p>\n<\/p>\n<h2 class=\"wp-block-heading\" id=\"h-related-for-kids\">Related For Kids<\/h2>\n<p><a href=\"https:\/\/spaceplace.nasa.gov\/james-webb-space-telescope\/en\/\"  rel=\"noreferrer noopener\"><strong>What is the Webb Telescope?<\/strong><\/a><\/p>\n<p><a href=\"https:\/\/spaceplace.nasa.gov\/\"  rel=\"noreferrer noopener\"><strong>SpacePlace for Kids<\/strong><\/a><\/p>\n<\/p>\n<h2 class=\"wp-block-heading\" id=\"h-en-espanol\">En Espa\u00f1ol<\/h2>\n<p><a href=\"https:\/\/ciencia.nasa.gov\/\"  rel=\"noreferrer noopener\"><strong>Ciencia de la NASA<\/strong><\/a><\/p>\n<p><a href=\"https:\/\/www.nasa.gov\/es\/\"  rel=\"noreferrer noopener\"><strong>NASA en espa\u00f1ol\u00a0<\/strong><\/a><\/p>\n<p><a href=\"https:\/\/spaceplace.nasa.gov\/sp\/\"  rel=\"noreferrer noopener\"><strong>Space Place\u00a0para ni\u00f1os<\/strong><\/a><\/p>\n<div id=\"\" class=\"hds-topic-cards nasa-gb-align-full maxw-full width-full padding-y-6 padding-x-3 color-mode-dark hds-module hds-module-full wp-block-nasa-blocks-topic-cards\">\n<div class=\"grid-container grid-container-block-lg padding-x-0\">\n<div class=\"grid-row flex-align-center margin-bottom-3\">\n<div class=\"desktop:grid-col-8 margin-bottom-2 desktop:margin-bottom-0\">\n<div class=\"label color-carbon-60 margin-bottom-2\">Keep Exploring<\/div>\n<h2 class=\"heading-36 line-height-sm\">Related Topics<\/h2>\n<\/p>\n<\/div>\n<\/div>\n<div class=\"grid-row grid-gap-2 hds-topic-cards-wrapper\">\n\t\t\t\t\t<a href=\"https:\/\/science.nasa.gov\/james-webb-space-telescope\/\" class=\"mobile:grid-col-12 tablet:grid-col-6 desktop:grid-col-3 topic-card margin-bottom-4 desktop:margin-bottom-0\" rel=\"noopener\"><\/p>\n<div class=\"hds-topic-card hds-cover-wrapper cover-hover-zoom bg-carbon-black\">\n<div class=\"skrim-overlay skrim-overlay-dark skrim-left mobile-skrim-top padding-3 display-flex flex-align-end flex-justify-start z-200\">\n<div>\n<h3 class=\"hds-topic-card-heading heading-29 color-spacesuit-white line-height-sm margin-top-0 margin-bottom-1\">\n\t\t\t\t\t\t\t\t<span>James Webb Space Telescope<\/span><br \/>\n\t\t\t\t\t\t\t\t<svg viewBox=\"0 0 32 32\" fill=\"none\" xmlns=\"http:\/\/www.w3.org\/2000\/svg\"><circle class=\"color-nasa-red\" cx=\"16\" cy=\"16\" r=\"16\"><\/circle><path d=\"M8 16.956h12.604l-3.844 4.106 1.252 1.338L24 16l-5.988-6.4-1.252 1.338 3.844 4.106H8v1.912z\" class=\"color-spacesuit-white\"><\/path><\/svg><br \/>\n\t\t\t\t\t\t\t<\/h3>\n<p class=\"margin-bottom-0 margin-top-2 color-carbon-20-important\">Webb is the premier observatory of the next decade, serving thousands of astronomers worldwide. It studies every phase in the\u2026<\/p>\n<\/p>\n<\/div>\n<\/div>\n<figure class=\"hds-media-background  \"><img loading=\"lazy\" decoding=\"async\" width=\"1536\" height=\"890\" src=\"https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/03\/main-image-star-forming-region-carina-nircam-final-5mb-1-jpeg.webp?w=1536\" class=\"attachment-1536x1536 size-1536x1536\" alt=\"\" style=\"transform: scale(1); transform-origin: 50% 50%; object-position: 50% 50%; object-fit: cover;\" block_context=\"nasa-block\" srcset=\"https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/03\/main-image-star-forming-region-carina-nircam-final-5mb-1-jpeg.webp 3600w, https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/03\/main-image-star-forming-region-carina-nircam-final-5mb-1-jpeg.webp?resize=300,174 300w, https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/03\/main-image-star-forming-region-carina-nircam-final-5mb-1-jpeg.webp?resize=768,445 768w, https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/03\/main-image-star-forming-region-carina-nircam-final-5mb-1-jpeg.webp?resize=1024,593 1024w, https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/03\/main-image-star-forming-region-carina-nircam-final-5mb-1-jpeg.webp?resize=1536,890 1536w, https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/03\/main-image-star-forming-region-carina-nircam-final-5mb-1-jpeg.webp?resize=2048,1186 2048w, https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/03\/main-image-star-forming-region-carina-nircam-final-5mb-1-jpeg.webp?resize=400,232 400w, https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/03\/main-image-star-forming-region-carina-nircam-final-5mb-1-jpeg.webp?resize=600,348 600w, https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/03\/main-image-star-forming-region-carina-nircam-final-5mb-1-jpeg.webp?resize=900,521 900w, https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/03\/main-image-star-forming-region-carina-nircam-final-5mb-1-jpeg.webp?resize=1200,695 1200w, https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/03\/main-image-star-forming-region-carina-nircam-final-5mb-1-jpeg.webp?resize=2000,1158 2000w\" sizes=\"auto, (max-width: 1536px) 100vw, 1536px\" \/><\/figure>\n<\/p>\n<\/div>\n<p>\t\t\t<\/a><br \/>\n\t\t\t\t\t<a href=\"https:\/\/science.nasa.gov\/universe\/\" class=\"mobile:grid-col-12 tablet:grid-col-6 desktop:grid-col-3 topic-card margin-bottom-4 desktop:margin-bottom-0\" rel=\"noopener\"><\/p>\n<div class=\"hds-topic-card hds-cover-wrapper cover-hover-zoom bg-carbon-black\">\n<div class=\"skrim-overlay skrim-overlay-dark skrim-left mobile-skrim-top padding-3 display-flex flex-align-end flex-justify-start z-200\">\n<div>\n<p class=\"hds-topic-card-heading heading-29 color-spacesuit-white line-height-sm margin-top-0 margin-bottom-1\">\n\t\t\t\t\t\t\t\t<span>Universe<\/span><br \/>\n\t\t\t\t\t\t\t\t<svg viewBox=\"0 0 32 32\" fill=\"none\" xmlns=\"http:\/\/www.w3.org\/2000\/svg\"><circle class=\"color-nasa-red\" cx=\"16\" cy=\"16\" r=\"16\"><\/circle><path d=\"M8 16.956h12.604l-3.844 4.106 1.252 1.338L24 16l-5.988-6.4-1.252 1.338 3.844 4.106H8v1.912z\" class=\"color-spacesuit-white\"><\/path><\/svg>\n\t\t\t\t\t\t\t<\/p>\n<\/p>\n<\/div>\n<\/div>\n<figure class=\"hds-media-background  \"><img loading=\"lazy\" decoding=\"async\" width=\"1536\" height=\"1514\" src=\"https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/09\/ngc5068-1-flat-final.jpg?w=1536\" class=\"attachment-1536x1536 size-1536x1536\" alt=\"\" style=\"transform: scale(1); transform-origin: 50% 50%; object-position: 50% 50%; object-fit: cover;\" block_context=\"nasa-block\" srcset=\"https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/09\/ngc5068-1-flat-final.jpg 3941w, https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/09\/ngc5068-1-flat-final.jpg?resize=300,296 300w, https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/09\/ngc5068-1-flat-final.jpg?resize=768,757 768w, https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/09\/ngc5068-1-flat-final.jpg?resize=1024,1009 1024w, https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/09\/ngc5068-1-flat-final.jpg?resize=1536,1514 1536w, https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/09\/ngc5068-1-flat-final.jpg?resize=2048,2019 2048w, https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/09\/ngc5068-1-flat-final.jpg?resize=50,50 50w, https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/09\/ngc5068-1-flat-final.jpg?resize=100,100 100w, https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/09\/ngc5068-1-flat-final.jpg?resize=400,394 400w, https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/09\/ngc5068-1-flat-final.jpg?resize=600,591 600w, https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/09\/ngc5068-1-flat-final.jpg?resize=900,887 900w, https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/09\/ngc5068-1-flat-final.jpg?resize=1200,1183 1200w, https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/09\/ngc5068-1-flat-final.jpg?resize=2000,1972 2000w\" sizes=\"auto, (max-width: 1536px) 100vw, 1536px\" \/><\/figure>\n<\/p>\n<\/div>\n<p>\t\t\t<\/a><br \/>\n\t\t\t\t\t<a href=\"https:\/\/science.nasa.gov\/universe\/stories\/\" class=\"mobile:grid-col-12 tablet:grid-col-6 desktop:grid-col-3 topic-card margin-bottom-4 desktop:margin-bottom-0\" rel=\"noopener\"><\/p>\n<div class=\"hds-topic-card hds-cover-wrapper cover-hover-zoom bg-carbon-black\">\n<div class=\"skrim-overlay skrim-overlay-dark skrim-left mobile-skrim-top padding-3 display-flex flex-align-end flex-justify-start z-200\">\n<div>\n<p class=\"hds-topic-card-heading heading-29 color-spacesuit-white line-height-sm margin-top-0 margin-bottom-1\">\n\t\t\t\t\t\t\t\t<span>Universe Stories<\/span><br \/>\n\t\t\t\t\t\t\t\t<svg viewBox=\"0 0 32 32\" fill=\"none\" xmlns=\"http:\/\/www.w3.org\/2000\/svg\"><circle class=\"color-nasa-red\" cx=\"16\" cy=\"16\" r=\"16\"><\/circle><path d=\"M8 16.956h12.604l-3.844 4.106 1.252 1.338L24 16l-5.988-6.4-1.252 1.338 3.844 4.106H8v1.912z\" class=\"color-spacesuit-white\"><\/path><\/svg>\n\t\t\t\t\t\t\t<\/p>\n<\/p>\n<\/div>\n<\/div>\n<figure class=\"hds-media-background  \"><img loading=\"lazy\" decoding=\"async\" width=\"1600\" height=\"500\" src=\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/astro\/universe\/2023\/09\/diagram_still_hi_res_122019.webp?w=1600&#038;h=500&#038;%23038;fit=clip&#038;%23038;crop=faces%2Cfocalpoint\" class=\"attachment-1536x1536 size-1536x1536\" alt=\"\" style=\"transform: scale(1); transform-origin: 50% 50%; object-position: 50% 50%; object-fit: cover;\" block_context=\"nasa-block\" srcset=\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/astro\/universe\/2023\/09\/diagram_still_hi_res_122019.webp?w=1600&#038;h=500&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1600w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/astro\/universe\/2023\/09\/diagram_still_hi_res_122019.webp?w=300&#038;h=94&#038;fit=crop&#038;crop=faces%2Cfocalpoint 300w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/astro\/universe\/2023\/09\/diagram_still_hi_res_122019.webp?w=768&#038;h=240&#038;fit=crop&#038;crop=faces%2Cfocalpoint 768w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/astro\/universe\/2023\/09\/diagram_still_hi_res_122019.webp?w=1024&#038;h=320&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1024w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/astro\/universe\/2023\/09\/diagram_still_hi_res_122019.webp?w=1536&#038;h=480&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1536w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/astro\/universe\/2023\/09\/diagram_still_hi_res_122019.webp?w=400&#038;h=125&#038;fit=crop&#038;crop=faces%2Cfocalpoint 400w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/astro\/universe\/2023\/09\/diagram_still_hi_res_122019.webp?w=600&#038;h=188&#038;fit=crop&#038;crop=faces%2Cfocalpoint 600w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/astro\/universe\/2023\/09\/diagram_still_hi_res_122019.webp?w=900&#038;h=281&#038;fit=crop&#038;crop=faces%2Cfocalpoint 900w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/astro\/universe\/2023\/09\/diagram_still_hi_res_122019.webp?w=1200&#038;h=375&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1200w\" sizes=\"auto, (max-width: 1600px) 100vw, 1600px\" \/><\/figure>\n<\/p>\n<\/div>\n<p>\t\t\t<\/a><br \/>\n\t\t\t\t\t<a href=\"https:\/\/science.nasa.gov\/mission\/roman-space-telescope\/exoplanets\/\" class=\"mobile:grid-col-12 tablet:grid-col-6 desktop:grid-col-3 topic-card margin-bottom-4 desktop:margin-bottom-0\" rel=\"noopener\"><\/p>\n<div class=\"hds-topic-card hds-cover-wrapper cover-hover-zoom bg-carbon-black\">\n<div class=\"skrim-overlay skrim-overlay-dark skrim-left mobile-skrim-top padding-3 display-flex flex-align-end flex-justify-start z-200\">\n<div>\n<p class=\"hds-topic-card-heading heading-29 color-spacesuit-white line-height-sm margin-top-0 margin-bottom-1\">\n\t\t\t\t\t\t\t\t<span>Exoplanets<\/span><br \/>\n\t\t\t\t\t\t\t\t<svg viewBox=\"0 0 32 32\" fill=\"none\" xmlns=\"http:\/\/www.w3.org\/2000\/svg\"><circle class=\"color-nasa-red\" cx=\"16\" cy=\"16\" r=\"16\"><\/circle><path d=\"M8 16.956h12.604l-3.844 4.106 1.252 1.338L24 16l-5.988-6.4-1.252 1.338 3.844 4.106H8v1.912z\" class=\"color-spacesuit-white\"><\/path><\/svg>\n\t\t\t\t\t\t\t<\/p>\n<\/p>\n<\/div>\n<\/div>\n<figure class=\"hds-media-background  \"><img loading=\"lazy\" decoding=\"async\" width=\"1536\" height=\"864\" src=\"https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/10\/exoplanets1.jpg?w=1536\" class=\"attachment-1536x1536 size-1536x1536\" alt=\"\" style=\"transform: scale(1); transform-origin: 50% 50%; object-position: 50% 50%; object-fit: cover;\" block_context=\"nasa-block\" srcset=\"https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/10\/exoplanets1.jpg 1920w, https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/10\/exoplanets1.jpg?resize=300,169 300w, https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/10\/exoplanets1.jpg?resize=768,432 768w, https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/10\/exoplanets1.jpg?resize=1024,576 1024w, https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/10\/exoplanets1.jpg?resize=1536,864 1536w, https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/10\/exoplanets1.jpg?resize=400,225 400w, https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/10\/exoplanets1.jpg?resize=600,338 600w, https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/10\/exoplanets1.jpg?resize=900,506 900w, https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/10\/exoplanets1.jpg?resize=1200,675 1200w\" sizes=\"auto, (max-width: 1536px) 100vw, 1536px\" \/><\/figure>\n<\/p>\n<\/div>\n<p>\t\t\t<\/a>\n\t\t\t\t<\/div>\n<\/p>\n<\/div>\n<\/div>\n","protected":false},"excerpt":{"rendered":"<p>An international team of researchers has discovered that previously observed variations in brightness of a free-floating planetary-mass object known as SIMP 0136 must be the result of a complex combination of atmospheric factors, and cannot be explained by clouds alone. Using NASA\u2019s James Webb Space Telescope to monitor a broad spectrum of infrared light emitted [\u2026]<\/p>\n","protected":false},"author":24,"featured_media":1,"comment_status":"open","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"om_disable_all_campaigns":false,"_monsterinsights_skip_tracking":false,"_monsterinsights_sitenote_active":false,"_monsterinsights_sitenote_note":"","_monsterinsights_sitenote_category":0,"_uf_show_specific_survey":0,"_uf_disable_surveys":false,"footnotes":""},"categories":[15612,15635,15636,15614,15637,15597,15638],"tags":[],"class_list":["post-181941","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-astrophysics","category-brown-dwarfs","category-exoplanets","category-goddard-space-flight-center","category-james-webb-space-telescope-jwst","category-science-research","category-the-universe"],"aioseo_notices":[],"_links":{"self":[{"href":"https:\/\/www.vibewire.com.au\/index.php?rest_route=\/wp\/v2\/posts\/181941","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.vibewire.com.au\/index.php?rest_route=\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.vibewire.com.au\/index.php?rest_route=\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/www.vibewire.com.au\/index.php?rest_route=\/wp\/v2\/users\/24"}],"replies":[{"embeddable":true,"href":"https:\/\/www.vibewire.com.au\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=181941"}],"version-history":[{"count":3,"href":"https:\/\/www.vibewire.com.au\/index.php?rest_route=\/wp\/v2\/posts\/181941\/revisions"}],"predecessor-version":[{"id":182027,"href":"https:\/\/www.vibewire.com.au\/index.php?rest_route=\/wp\/v2\/posts\/181941\/revisions\/182027"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/www.vibewire.com.au\/index.php?rest_route=\/"}],"wp:attachment":[{"href":"https:\/\/www.vibewire.com.au\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=181941"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.vibewire.com.au\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=181941"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.vibewire.com.au\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=181941"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}