Rubin observatory finds huge asteroid spinning impossibly fast

The Vera C. Rubin Observatory in Chile has detected a 710-metre-wide asteroid that rotates once every 1.9 minutes, faster than previously thought possible for its size. Named 2025 MN45, it is the quickest-spinning asteroid over 500 metres across ever observed. Astronomers say its speed suggests it is a single solid rock or even metal, not a loose rubble pile.

Astronomers using the Vera C. Rubin Observatory in Chile identified the asteroid 2025 MN45 during its first nine nights of observations in late April and early May 2025. Dmitrii Vavilov at the University of Washington in Seattle and his colleagues analysed the data, spotting 76 asteroids with reliable rotational periods. Of these, 19 were super-fast rotators, spinning once every 2.2 hours or faster—the supposed limit for rubble pile asteroids held together only by gravity. The fastest among them rotates every 13 minutes or so. They also found three ultra-fast rotators with periods of 3.8 minutes, 1.92 minutes, and 1.88 minutes. The standout is 2025 MN45, measuring about 710 metres across and spinning every 1.92 minutes—faster than any known asteroid larger than 500 metres. Vavilov presented these findings at the Lunar and Planetary Science Conference in Texas on 17 March. Initially, the team did not search for rotations under 5 minutes. “We thought that was crazy that they could rotate any faster,” Vavilov said. He added, “2.2 hours is supposed to be the limit for this asteroid, and yet it’s rotating in less than 2 minutes.” Its extreme speed rules out a rubble pile structure. “Even clay would not be enough to hold this asteroid together, so it’s probably one big rock or even solid metal,” Vavilov explained. The observatory's 10-year survey of the southern sky is expected to reveal more such asteroids, highlighting their diversity. The research appears in The Astrophysical Journal Letters (DOI: 10.3847/2041-8213/ae2a30).

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Artistic rendering of the James Webb Space Telescope observing the atmosphere-shrouded molten super-Earth TOI-561 b near its host star.
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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.

Researchers from Columbia University have identified a potential millisecond pulsar spinning every 8.19 milliseconds close to Sagittarius A*, the supermassive black hole at the Milky Way's center. This discovery, part of the Breakthrough Listen Galactic Center Survey, could provide insights into space-time under extreme gravity if confirmed. The findings were published in The Astrophysical Journal.

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An international team led by the University of Oxford has discovered one of the largest rotating structures in the universe, a thin chain of galaxies spinning in sync within a larger cosmic filament. Located about 140 million light years from Earth, this structure challenges models of galaxy formation. The findings, published in Monthly Notices of the Royal Astronomical Society, suggest that large-scale cosmic structures influence galaxy spin.

New research shows that Nasa's Dart spacecraft, which crashed into the asteroid moonlet Dimorphos in 2022, has changed the orbit of the binary asteroid system around the sun. This marks the first time a human-made object has measurably altered a celestial body's path in this way. The findings highlight potential methods for planetary defense against hazardous space objects.

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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 using the Hubble Space Telescope observed comet C/2025 K1 (ATLAS) shortly after it split into four fragments, thanks to a lucky scheduling change. The high-resolution images provide unprecedented detail on the event. Researchers noted an unexpected delay in the comet's brightening after the breakup.

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Scientists have analyzed rare carbonaceous chondrites to uncover the composition of carbon-rich asteroids, identifying potential resources for future space exploration. The study, led by researchers at the Institute of Space Sciences, suggests certain asteroid types could yield water and materials, though large-scale mining remains challenging. Published in the Monthly Notices of the Royal Astronomical Society, the findings highlight promising targets for missions to the Moon and Mars.

 

 

 

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