In a groundbreaking discovery, NASA's James Webb Space Telescope (JWST) has revealed intriguing details about a distant exoplanet, sparking a debate among scientists about its potential habitability. The exoplanet, known as TOI-270 d, lies approximately 70 light-years away and boasts twice the radius of Earth.
Observations from the James Webb Space Telescope exposed the presence of water vapour, methane, and carbon dioxide in the exoplanet's atmosphere, suggesting a composition consistent with a colossal water world. Researchers from the University of Cambridge propose that an entire surface ocean, potentially reaching temperatures exceeding 100 degrees Celsius, envelops TOI-270 d. However, they caution against envisioning this as an inviting seascape, emphasizing the extreme conditions, The Guardian reported.
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Astronomers remain divided on the habitability of TOI-270 d. A Canadian team, conducting additional observations of the same exoplanet, disputes the water world hypothesis. They argue that the planet might be too hot, reaching temperatures as high as 4,000 degrees Celsius, featuring a rocky surface beneath an incredibly dense atmosphere of hydrogen and water vapour.
Regardless of the ongoing debate, these findings underscore the unprecedented insights offered by the James Webb Telescope into the nature of planets beyond our solar system. By analyzing starlight filtered through planetary atmospheres, astronomers can decipher detailed chemical compositions, aiding in understanding surface conditions and the potential for extraterrestrial life.
The absence of ammonia in TOI-270 d's atmosphere forms the basis for the water ocean hypothesis, as basic chemistry predicts its depletion in a hydrogen-rich atmosphere due to its solubility in water. This leads to the intriguing concept of a 'hycean' world, with a water ocean beneath a hydrogen-rich atmosphere.
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