New images reveal Betelgeuse’s buddy star
A small member of our solar system out beyond Pluto may be shrouded in a thin layer of gas. If so, it would be the first object of its size — and the most remote rock in our solar system — known to host even a wispy atmosphere.
“This discovery suggests that small icy worlds beyond Neptune may not be as inactive or unchanging as we often assumed,” says Ko Arimatsu. “Until now, Pluto was the only [object beyond Neptune] with a confirmed atmosphere.”
Arimatsu is an astronomer at the National Astronomical Observatory of Japan. It’s in Mitaka. His group shared the new finding May 4 in Nature Astronomy.
Arimatsu’s group tracked the object — known as 2002 XV93 — with a network of telescopes in Japan. On January 10, 2024, those telescopes saw it move in front of a distant star. Such tiny eclipses are called occultations (Ah-kul-TAY-shuns). They can reveal whether some object in our solar system hosts an atmosphere.
If 2002 XV93 were bare, the star behind it would have seemed to blink out and reappear sharply. But Arimatsu and his teammates saw the star’s light gradually fade and reappear over about 1.5 seconds. That smooth dimming is best explained by starlight passing through a layer of gas. Those data suggest this thin atmosphere has a pressure about one ten-millionth that of Earth’s.
“I was genuinely surprised,” Arimatsu says. The object is about 470 kilometers (290 miles) wide. The Grand Canyon is about that long. At such a small size, 2002 XV93’s gravity should be too weak to hold on to a gas for long. So its atmosphere should have vanished long ago, unless something has added new gas to it.
Perhaps an icy body like a comet recently smashed into 2002 XV93. That could have released a plume of gas around the object. Or maybe 2002 XV93 releases gas regularly from icy volcanoes on its surface.
The astronomers can’t be certain what’s going on just from viewing 2002 XV93 pass in front of one star. The data couldn’t show what the atmosphere is made of. So the small body might even be swaddled in dust, not gas, Arimatsu notes. Nor could they show how high above the body’s surface any atmosphere extends.
“Future observations will be important,” he says. Say its atmosphere fades over the next few years. That could mean he had detected a plume kicked up by an impact. If it sticks around or varies over time, that might make a case for surface volcanoes.
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For the first time, humankind has changed a space rock’s orbit around the sun.
Four years ago, NASA rammed its DART spacecraft into the asteroid Dimorphos. The goal was to see if a space probe could change an asteroid’s motion. Why? It could be useful if a big rock were ever headed for Earth.
Soon after the crash, it was clear that DART had knocked its asteroid closer to Didymos, an even bigger rock that it orbits. Now, NASA reports that the smashup had an even bigger impact. It changed the asteroid duo’s speed as they orbit the sun together.
DART’s crash landing slowed the asteroid pair by 10 micrometers per second. That might not sound like much. But tweaking the motions of space rocks millions of kilometers (miles) from Earth is a huge deal. It could inform plans for shielding our planet from future asteroid strikes.
Researchers shared the findings March 6 in Science Advances.
DART is short for Double Asteroid Redirection Test. The initial goal had been to simply nudge Dimorphos into a tighter orbit around Didymos. Mission leaders aimed to cut 73 seconds off Dimorphos’ nearly 12-hour path around its partner. In reality, the crash shortened Dimorphos’ orbit around Didymos by 32 minutes.
Most of that change came from the impact itself. Like giving the asteroid a big shove, the spacecraft pushed Dimorphos closer to Didymos. The crash also blasted rocks off Dimorphos’ surface. The motion of that flying debris gave the asteroid an extra kick.
But some of the debris knocked off Dimorphos didn’t just leave that space rock. It escaped the gravity of the two-asteroid system altogether. That escaping debris took some momentum away from the duo. As a result, their joint motion around the sun changed, reports Rahil Makadia. He studies planetary defense at the University of Illinois in Urbana–Champaign.
To figure out how much the asteroids’ motion changed, astronomers watched the rocks pass in front of distant stars. As the asteroids passed by, they dimmed some of the stars’ light — like tiny eclipses. These blinks can be seen only from specific locations, which can fall anywhere on Earth.
Astronomers could predict when Dimorphos and Didymos should pass in front of stars, based on their old path around the sun. By comparing those predictions to observations, they could see how much the asteroids’ path changed after DART’s hit.
Between October 2022 and March 2025, Makadia and the team gathered 22 such measurements. Amateur astronomers provided a lot of these data, Makadia says. “There was an observer who drove two days each way into the Australian outback to get these measurements.”
The asteroids’ orbit around the sun was about 150 milliseconds longer than before the DART impact, the new data show.
The European Space Agency’s Hera spacecraft will reach Didymos and Dimorphos later this year. When it does, the spacecraft could confirm the asteroids’ new orbit.
Didymos and Dimorphos were not a threat to Earth before DART. They aren’t now, either. But knowing how an impact changes one asteroid’s orbit can help figure out how to defend Earth from a dangerously big incoming space rock. That’s crucial, Makadia says, “in case we need to [deflect an asteroid] for real.”
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