Webb lifts veil on common but mysterious type of exoplanet
- In 2025, NASA's James Webb Space Telescope studied TOI-421 b, a scorching sub-Neptune-sized planet orbiting a star similar to the Sun.
- Scientists targeted TOI-421 b due to its high temperature of about 1,340°F and previous expectations of a clear atmosphere with little haze.
- The team detected water vapor, sulfur dioxide, and possible carbon monoxide in TOI-421 b's hydrogen-rich atmosphere while confirming the absence of methane and carbon dioxide.
- Brian Davenport explained that by analyzing the patterns in the light spectrum, they identified different gases present, which enabled them to figure out the atmosphere's composition, revealing an unexpected dominance of hydrogen.
- These results indicate that TOI-421 b likely experienced a distinct formation and evolutionary process compared to cooler sub-Neptune planets, highlighting the need for further investigation to determine if this characteristic is common among hot sub-Neptunes.
11 Articles
11 Articles
The Most Common Type of Exoplanet Was Difficult To Observe Until the JWST Came Along
The idea that our Solar System is representative of other solar systems hasn't survived the age of exoplanet discovery. Kepler and TESS have shown us that our system doesn't even contain the most common type of planet: sub-Neptunes. These planets pose a mystery to planetary scientists, and the JWST is helping unravel the mystery.
Webb lifts veil on common but mysterious type of exoplanet
Though they don't orbit around our sun, sub-Neptunes are the most common type of exoplanet, or planet outside our solar system, that have been observed in our galaxy. These small, gassy planets are shrouded in mystery…and often, a lot of haze. Now, by observing exoplanet TOI-421 b, NASA's James Webb Space Telescope is helping scientists understand sub-Neptunes in a way that was not possible prior to the telescope's launch.
Hot sub-Neptune Exoplanet TOI-421 b NIRISS/NIRSpec Transmission Spectrum - Astrobiology
This is a transmission spectrum captured by the NASA/ESA/CSA James Webb Space Telescope that reveals the presence of water (H2O) and the possible presence of sulfur dioxide (SO2) and carbon monoxide (CO), but no signs of carbon dioxide (CO2) or methane (CH4), in the atmosphere of the hot sub-Neptune exoplanet TOI-421 b. The observations support […] The post Hot sub-Neptune Exoplanet TOI-421 b NIRISS/NIRSpec Transmission Spectrum appeared first o…
Webb Reveals the Atmospheric Structure of Sub-Neptune TOI
Subneptin is a type of exoplanet characterized by high birth discharge thrombosis and lacks analogs within our solar system. Significantly smaller than gas giants, and typically cooler than Hot Jupiter exoplanets, these worlds were notably challenging to study before the launch of the NASA/ESA/CSA James Webb Space Telescope. Many subneptins are obscured by thick clouds [...] Source The post Webb Reveals the Atmospheric Structure of Sub-Neptune T…
Webb Determines Atmospheric Makeup of Sub-Neptune TOI
Astronomers using Webb have captured the transmission spectrum of the sub-Neptune TOI-421b and uncovered the chemical fingerprints of its atmosphere. The post Webb Determines Atmospheric Makeup of Sub-Neptune TOI-421b appeared first on Sci.News: Breaking Science News.
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