March 17, 2025

Huh? James Webb telescope spots ‘rogue’ planet with cake-like atmosphere – Livescience.com

This artist’s concept shows what the isolated planetary-mass object SIMP 0136 could look like based on recent observations from the NASA/ESA/CSA James Webb Space Telescope. SIMP 0136 has a mass about 13 times that of Jupiter. Although it is thought to have the structure and composition of a gas giant, it is not technically classified as an exoplanet because it doesn’t orbit its own star. The colors shown in the illustration represent near-infrared light, which is invisible to human eyes. SIMP 0136 is relatively warm — about 825 degrees Celsius or 1,100 kelvins — but is not hot enough to give off enough visible light to see from Earth, and is not illuminated by a host star. The bluish glow near the poles represents auroral energy (light given off by electrons spiraling in a magnetic field) which has been detected at radio wavelengths. Researchers used NIRSpec (Near-infrared Spectrograph) and MIRI (Mid-Infrared Instrument) to monitor the brightness of SIMP 0136 over two full rotations in July 2023. By analyzing the change in brightness of different wavelengths over time, researchers were able to detect variability in cloud cover at different depths, temperature variations in the high atmosphere, and changes in carbon chemistry as different sides of the object rotated in and out of view. SIMP 0136 is located within the Milky Way, about 20 light-years from Earth, in the constellation Pisces. It is the brightest isolated planet or brown dwarf visible from the Northern Hemisphere, and is thought to be about 200 million years old. This illustration is based on spectroscopic observations. Webb has not captured a direct image of the object. [Image description: Illustration of a gas giant planet or brown dwarf on a background of distant stars.]

The James Webb Space Telescope has spotted a ‘rogue’ cosmic object barrelling through our galaxy without a star, and covered in clouds of iron and magnesium minerals.
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Using the James Webb Space Telescope (JWST), researchers have generated the first-ever weather report of a rogue exoplanet-like object — and it shows patches of clouds and carbon chemicals, along with high-altitude auroras.The findings, published March 3 in The Astrophysical Journal Letters, also revealed that the celestial object possesses a complex, layered atmosphere.Earth’s atmosphere is a blanket of gases, primarily nitrogen and oxygen. But other planets in the solar system have very different atmospheres. For example, Venus’ air is much thicker than Earth’s and is vitriolic: it’s made of sulfuric acid. This diversity of atmospheres has also been observed in planets beyond our cosmic neighborhood: Some exoplanets have water vapor-soaked atmospheres, while others host superheated clouds of sand.Now, researchers have pointed JWST at a mysterious object called SIMP 0136+0933 to learn more about its atmosphere. This object’s identity is still nebulous, said study lead author Allison McCarthy, a graduate student in Boston University’s astronomy department.”[I]t’s not a planet in the traditional sense — since it doesn’t orbit a star,” she told Live Science in an email. However, “it also has a lower mass than a typical brown dwarf [a so-called ‘failed star’],” she added.Related: 32 alien planets that really existSIMP 0136+0933 has a 2.4-hour-long day and is located in the Carina Nebula 20 light-years away. Because it is the brightest free-floating planetary-mass object in the Northern Hemisphere and is far from stars that could obfuscate observations, it has been directly photographed by telescopes like NASA’s Spitzer Space Telescope. These observations revealed that SIMP 0136+0933 has an unusually variable atmosphere, with fluctuations in the electromagnetic spectrum’s infrared region (which humans would perceive as heat). But the physical phenomena causing this variability were still unknown.Get the world’s most fascinating discoveries delivered straight to your inbox.To unravel these processes, McCarthy and colleagues used JWST’s Near-Infrared Spectrograph to measure the intensity of the short-wave radiation SIMP 0136+0933 emitted. They collected about 6,000 such datasets over nearly three hours on July 23, 2023, sampling data from the whole object. Then, over the next three hours, they repeated the process for longer wavelengths, using the space telescope’s Mid-Infrared Instrument.The researchers then created light curves to show how the infrared radiation’s “brightness” (or intensity) changed over time. These curves revealed that different wavelengths behaved differently. At any one point, some brightened, others dimmed and others didn’t change. Despite this, the researchers found the light curves formed three clusters, each with a specific — albeit somewhat variable — shape.The similar light-curve shapes suggested that similar atmospheric mechanisms were causing them. To determine these, the researchers built models of SIMP 0136+0933’s atmosphere. This enabled them to infer that the first wavelength cluster originated from a low-lying layer of iron clouds, with the second cluster coming from higher-lying clouds of forsterite, a magnesium mineral. The cloud layers were also probably patchy, which could have caused some of the variability in the wavelength clusters’ curves.But clouds couldn’t explain the third wavelength cluster, which seemed to originate high above them. Instead, the researchers believe this radiation came from “hotspots,” or hot pockets of the atmosphere that may originate from radio auroras. These radio auroras resemble Earth’s northern lights, but they’re in the radio-wavelength range.—Surprise discovery in alien planet’s atmosphere could upend decades of planet formation theory—Exoplanet with iron rain has violent winds ‘like something out of science fiction’—Nearby exoplanet has grown a tail 44 times longer than Earth — and it is acting like a giant ‘stellar windsock’Yet even these models couldn’t explain all of the observations, like why the first cluster’s curves had such diverse shapes. The researchers proposed that clumps of carbon-based chemicals, such as carbon monoxide, in the atmosphere may have been responsible, absorbing radiation at some wavelengths at certain times.”While these variability mechanisms had been hypothesized, this was the first time we observed them directly in SIMP 0136’s atmosphere,” McCarthy said. But a few hours of observations aren’t enough to understand SIMP 0136+0933’s atmosphere in the long term. For that, the researchers will need to study the object over several days, possibly with NASA’s Nancy Grace Roman Space Telescope, which is expected to launch in 2027.Abha Jain is a freelance science writer. She did a masters degree in biology, specializing in neuroscience, from the Indian Institute of Science, Bengaluru, India, and is almost through with a bachelor’s degree in archaeology from the University of Leicester, UK. She’s also a self-taught space enthusiast, and so loves writing about topics in astronomy, archaeology and neuroscience.Please logout and then login again, you will then be prompted to enter your display name.’Utterly cataclysmic’: James Webb telescope spots 2 alien planets disintegrating before our eyesExoplanet with iron rain has violent winds ‘like something out of science fiction’Why is it still so hard to make nuclear weapons?
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Source: https://www.livescience.com/space/exoplanets/james-webb-telescope-spots-a-strange-rogue-world-with-a-cake-like-atmosphere

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