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NASA's James Webb Space Telescope Discovers 'Forbidden Planet' TOI-5205b
Discovery of the 'Forbidden Planet' TOI-5205b
NASA's James Webb Space Telescope (JWST) has discovered a bizarre giant exoplanet, TOI-5205b, that challenges long-standing theories of planetary formation. This planet, which blocks about 6% of its host star's light, appears to be too massive to orbit such a small M-dwarf star, TOI-5205. This pairing is considered 'forbidden' under conventional models of planetary formation, as giant planets are not expected to form around such small stars.
Mystery of the Atmospheric Composition
Findings published in the Astronomical Journal reveal something shocking about TOI-5205b: its atmosphere is incredibly poor in heavy elements like carbon and oxygen. In fact, the planet possesses a lower 'metallicity' than its own host star. Astrophysicist Angeli Piet explained that this makes it stand out among all the giant planets studied to date. While spectroscopes detected methane and hydrogen sulfide, the overall carbon-rich, oxygen-poor environment is rarely observed, further deepening the mystery.
Testing the Limits of Planetary Science
Models suggest that TOI-5205b's overall internal composition is actually up to 100 times richer in heavy elements than its atmosphere. This implies that heavy materials likely sank deep into the planet's core during formation and stopped mixing with the outer atmospheric layers. This landmark study is part of the GEMS (Giant Exoplanet M-dwarf Survey) project, a broader initiative focusing on giant planets that orbit small, cool M-dwarf stars. These bizarre star systems are increasingly becoming the ultimate laboratories for testing the absolute limits of planetary science. Researchers also overcame the challenge of starspots on the host star, refining their correction techniques for TOI-5205b to pave the way for more accurate Webb observations in the future.
*Source: YouTube: WION (2026-05-07)*
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