Exoplanets
Webb telescope uncovers atmosphere on molten super-Earth TOI-561 b
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NASA's James Webb Space Telescope has detected signs of a thick atmosphere on the ultra-hot exoplanet TOI-561 b, challenging assumptions about such worlds. This rocky planet, orbiting its star in under 11 hours, shows lower temperatures and density than expected, suggesting a layer of gases above a magma ocean. The findings, published on December 11, highlight how intense radiation might not strip away all atmospheres from small, close-in planets.
A team led by Professor Lisa Kaltenegger at Cornell University has pinpointed 45 rocky exoplanets in the habitable zones of their stars, where liquid water might exist. The research, drawing on data from ESA's Gaia mission and NASA's Exoplanet Archive, highlights prime targets for the search for extraterrestrial life. Published in Monthly Notices of the Royal Astronomical Society, the study also notes 24 additional candidates in a stricter habitable zone.
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NASA's James Webb Space Telescope has observed an unusually thick haze on the exoplanet Kepler-51d, obscuring its atmospheric composition. This super-puff planet, part of a rare low-density system around the star Kepler-51, challenges standard models of planetary formation. The findings, led by Penn State researchers, were published on March 16 in the Astronomical Journal.
Astronomers have forecasted a rare alignment of two planets and their star in the Kepler-89 system for April 1, 2026, but the event may pass unobserved due to denied telescope access. This exosyzygy, first identified in 2010, offers a unique chance to study planetary orbits, yet complications in scheduling have thwarted observation efforts. Researchers remain optimistic about the prediction while planning for future opportunities.
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Scientists have directly measured the mass and distance of a free-floating planet drifting through the Milky Way, using simultaneous observations from Earth and space. The planet, with a mass similar to Saturn, likely formed around a star before being ejected into interstellar space. This discovery highlights new methods for studying these elusive objects.
Astronomers have discovered a companion star orbiting kappa Tucanae A that likely sustains a puzzling cloud of ultra-hot dust. Located 70 light-years from Earth, the dust endures extreme conditions near the main star, challenging previous understandings of planetary systems. This finding, achieved through advanced interferometry, could aid future searches for Earth-like exoplanets.
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Researchers at the University of Tokyo have developed a timing-based approach to distinguish how hot Jupiters migrated inward to their stars. By analyzing orbital circularization timescales, they identified about 30 such planets that likely moved peacefully through protoplanetary disks rather than via violent scattering. This finding provides clearer evidence of formation processes for these massive exoplanets.
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