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What's TOI-6894b that just showed up around a dwarf star only 2.5 times its size; here's why that's weird

What's TOI-6894b that just showed up around a dwarf star only 2.5 times its size; here's why that's weird

Economic Times07-06-2025
Reuters An artist's impression of a newly discovered giant planet named TOI-6894 b (top right) orbiting a red dwarf star (center) about 20% the mass of the sun, the image was released on June 4, 2025. University of Warwick/Mark Garlick/Handout via REUTERS NO RESALES. NO ARCHIVES. THIS IMAGE HAS BEEN SUPPLIED BY A THIRD PARTY
Astronomers have made a discovery that challenges long-standing beliefs about how planets form. A gas giant planet, roughly the size of Saturn, has been found orbiting an unusually small red dwarf star. This rare pairing defies current models, which say small stars don't have enough material in their surrounding disks to form such large planets.
Named TOI-6894b, the planet was found about 241 light-years from Earth in the constellation Leo. TOI-6894b is about 1.07 times the diameter of Saturn but has just over half its mass. This makes the planet very low in density, similar to that of a beach ball. Despite its large size, the planet orbits extremely close to its host star, completing a full revolution in just under three Earth days.
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The star it orbits, TOI-6894, is a red dwarf with only about 21% the mass of the Sun and roughly 250 times dimmer. In terms of physical size, the star is just 2.5 times wider than the planet itself, a remarkable size ratio rarely seen in planetary systems. The formation of such a large planet around such a small star has puzzled astronomers. According to the well-accepted 'core accretion' model, large planets are thought to grow from small rocky cores that gradually gather gas from the star's surrounding protoplanetary disk. But small, dim stars like red dwarfs are believed to have disks too thin and short-lived to form massive planets before the gas disappears.
Dr. Teruyuki Hirano, the lead researcher from the Graduate University for Advanced Studies in Japan, noted that this planetary system 'is completely inconsistent with what we thought we knew.' He said the discovery 'forces us to question our assumptions about planet formation.'
The planet was first flagged by NASA's Transiting Exoplanet Survey Satellite (TESS), which detects periodic dips in starlight caused by planets passing in front of their stars. Follow-up observations using the European Southern Observatory's Very Large Telescope (VLT) confirmed the planet's mass and orbit.
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More data will be needed to determine how TOI-6894b formed. Future observations by the James Webb Space Telescope could reveal more about its atmosphere and structure, including how much of it is made up of hydrogen and helium and whether it has a large core. Red dwarfs are the most common type of star in the Milky Way, making up about 75% of the stellar population. They're also seen as good candidates for hosting habitable planets due to their long lifespans. Discoveries like TOI-6894b suggest there's still much to learn about the diversity of planetary systems these stars may host.Though this is not the first time a massive planet has been found orbiting a small star, it is one of the most extreme examples yet.
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