Asteroids news, articles and features | èƵ /topic/asteroids/ Science news and science articles from èƵ Thu, 18 Jun 2026 10:45:54 +0000 en-US hourly 1 https://wordpress.org/?v=7.0.1 242057827 Dinosaur-killing asteroid impact site stayed hot for millions of years /article/2529627-dinosaur-killing-asteroid-impact-site-stayed-hot-for-millions-of-years/?utm_campaign=RSS|NSNS&utm_content=asteroids&utm_medium=RSS&utm_source=NSNS Tue, 09 Jun 2026 09:01:59 +0000 /?post_type=article&p=2529627
Illustration of the Chicxulub asteroid impact, which took place 66 million years ago
MARK GARLICK/Science Photo Library/Getty Images

The asteroid strike that wiped out the dinosaurs hit with such force that it took at least 8 million years for the impact site to cool down, creating a warm underground ecosystem where microscopic life thrived.

The Chicxulub asteroid, which collided with Earth 66 million years ago at what is now Mexico, is thought to have been as large as 15 kilometres in diameter. The strike caused so much climate chaos that it wiped out three-quarters of species on Earth. All the dinosaurs except the ancestors of birds became extinct and a nuclear winter gripped the planet for at least 15 years.

Its effects were also felt deep underground. “The Chicxulub impact was big enough to cause deformation at least 35 kilometres under the surface of the Earth, detectable using geophysical surveys,” says at the University of Glasgow, UK.

The impact melted about 10,000 cubic kilometres of rock, she says. The combination of melted rock and seawater created porous material filled with tiny pockets of hot water, known as a hydrothermal system.

Because of the presence of minerals that only form where there is liquid water and heat, we know that the asteroid would have created hydrothermal environments to depths of several kilometres. But the scale and lifespan of the heating and resulting hydrothermal system has, it seems, been massively underestimated.

Previously, it was thought it took only 2 million years for the impact site to cool down. Now, Pickersgill and her colleagues say it may have taken at least four times longer, giving hydrothermal life much more time to thrive.

“One of the biggest unknowns about all impact-generated hydrothermal systems, and Chicxulub in particular, is how long the heat keeps water circulating through the structure,” says Pickersgill.

To figure this out, the team drilled 1 kilometre into the crater to obtain rock cores. Because potassium in the rocks has decayed into argon gas over time, the researchers could measure the amount of argon trapped in the samples to find out their age.

“We got a range of ages from the time of impact at 66 million years ago to about 58 million years ago,” says Pickersgill. “That told us that hydrothermal activity was ongoing in at least part of the Chicxulub structure for 8 million years after the impact.”

Sulphur isotopes in the cores provide evidence that microbial life existed in the hydrothermal system and recovered rapidly after the impact.

The results mean that the very earliest impact craters on the young Earth – and perhaps other worlds – may also have had habitable hydrothermal systems for longer than previously known.

“This provides more opportunity for life to develop, evolve and spread,” says Pickersgill. “It supports the concept that early life on Earth may have found a long-term home in impact craters, and possibly even life on other planets where these massive impact craters are dominant surface features.”

at Curtin University in Perth, Australia, says while there is “not an entirely unambiguous record of continuous hydrothermal activity” at Chicxulub, the evidence is strong that the impact site stayed hot for millions of years.

“Large impacts do not simply destroy environments,” he says. “They can also create long-lived underground systems where hot fluids circulate through shattered rock. These chemically rich settings may provide sheltered habitats for microbes and perhaps even favourable conditions for some of the early chemical steps towards life.”

Journal reference:

Communications Earth & Environment

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Asteroid set to fly very close to Earth /article/2526328-asteroid-set-to-fly-very-close-to-earth/?utm_campaign=RSS|NSNS&utm_content=asteroids&utm_medium=RSS&utm_source=NSNS Wed, 13 May 2026 15:08:59 +0000 /?post_type=article&p=2526328 2526328 We could protect Earth from dangerous asteroids using a huge magnet /article/2520960-we-could-protect-earth-from-dangerous-asteroids-using-a-huge-magnet/?utm_campaign=RSS|NSNS&utm_content=asteroids&utm_medium=RSS&utm_source=NSNS Fri, 27 Mar 2026 11:00:55 +0000 /?post_type=article&p=2520960 2520960 We’ve spotted a huge asteroid spinning impossibly fast /article/2520088-weve-spotted-a-huge-asteroid-spinning-impossibly-fast/?utm_campaign=RSS|NSNS&utm_content=asteroids&utm_medium=RSS&utm_source=NSNS Fri, 20 Mar 2026 17:00:40 +0000 /?post_type=article&p=2520088 2520088 Private company to land on asteroid Apophis as it flies close to Earth /article/2520020-private-company-to-land-on-asteroid-apophis-as-it-flies-close-to-earth/?utm_campaign=RSS|NSNS&utm_content=asteroids&utm_medium=RSS&utm_source=NSNS Fri, 20 Mar 2026 14:52:28 +0000 /?post_type=article&p=2520020 2520020 The asteroid Ryugu has all of the main ingredients for life /article/2519423-the-asteroid-ryugu-has-all-of-the-main-ingredients-for-life/?utm_campaign=RSS|NSNS&utm_content=asteroids&utm_medium=RSS&utm_source=NSNS Mon, 16 Mar 2026 16:00:10 +0000 /?post_type=article&p=2519423 2519423 NASA changed an asteroid’s orbit around the sun for the first time /article/2518205-nasa-changed-an-asteroids-orbit-around-the-sun-for-the-first-time/?utm_campaign=RSS|NSNS&utm_content=asteroids&utm_medium=RSS&utm_source=NSNS Fri, 06 Mar 2026 19:00:00 +0000 /?post_type=article&p=2518205 2518205 How worried should you be about an asteroid smashing into Earth? /article/2517120-how-worried-should-you-be-about-an-asteroid-smashing-into-earth/?utm_campaign=RSS|NSNS&utm_content=asteroids&utm_medium=RSS&utm_source=NSNS Fri, 27 Feb 2026 10:38:31 +0000 /?post_type=article&p=2517120 2517120 Two asteroids crashed around a nearby star, solving a cosmic mystery /article/2509086-two-asteroids-crashed-around-a-nearby-star-solving-a-cosmic-mystery/?utm_campaign=RSS|NSNS&utm_content=asteroids&utm_medium=RSS&utm_source=NSNS Thu, 18 Dec 2025 19:00:49 +0000 /?post_type=article&p=2509086 A composite Hubble Space Telescope image of the dust belt around the bright star Fomalhaut
A composite image of the dust belt around Fomalhaut (obscured in the middle). In the inset, dust cloud cs1, imaged in 2012, is pictured with dust cloud cs2, imaged in 2023
NASA, ESA, Paul Kalas/UC Berkeley
Around the nearby star Fomalhaut, asteroids are smashing into each other in a series of cosmic cataclysms, creating huge clouds of dust. For the first time, astronomers are watching one of these collisions as it occurs, which could provide a window into the early days of our own solar system. Fomalhaut has a history of strange observations: in 2008, at the University of California, Berkeley, and his colleagues reported what seemed to be a giant planet in orbit around the young star, based on observations with the Hubble Space Telescope made in 2004 and 2005. Over the years, though, as more observations have rolled in, researchers have hotly debated over what this strange object, called Fomalhaut b, might be. It was either a planet a bit larger than Jupiter, or a cloud of debris. Now, Kalas and his team have used Hubble to look at Fomalhaut once again. “In 2023, we used the same instrument we’d used [before], and we did not detect Fomalhaut b – it wasn’t visible anymore,” says Kalas. “But what really shocked us was [that] there was a new Fomalhaut b.” This new bright spot, called Fomalhaut cs2 (short for “circumstellar source”), couldn’t be a planet, or it would have been seen sooner. The best explanation is that it is a cloud of dust created by the collision of two large asteroids, or planetesimals, each around 60 kilometres in diameter. The disappearance of Fomalhaut b hints that it was probably a similar dust cloud all along. “These sources are noisy and erratic, so we’re still some ways off a firm conclusion,” says at Columbia University. “But, all of the evidence to date seems to fit neatly under the umbrella explanation of collisions between proto-planets in a nascent system.” Spotting two such smash-ups is unexpected, though. “Theory dictates that you shouldn’t see these collisions except once every 100,000 years or rarer. And yet, for some reason, we’ve seen 2 events in 20 years,” says Kalas. “Fomalhaut is sparkling like a holiday tree, and that is a surprise.”
It may mean that collisions between planetesimals are more common than we had thought, at least around relatively young stars like Fomalhaut. Kalas and his colleagues have more observations scheduled over the next three years with both Hubble and the more powerful James Webb Space Telescope (JWST) to watch how Fomalhaut cs2 behaves moving forward and to try to find the now-dimmer Fomalhaut b. This is a unique opportunity to study these collisions in real time. “We no longer have to depend solely on theory to understand these violent impacts; we can actually see them,” says Kalas. More observations could teach us not just about young planetary systems in general, but also about our own early solar system and where it fits in the cosmic menagerie. “We’ve long wondered if the moon-forming impact was typical or not beyond our cosmic shore, and here we see compelling evidence that collisions are par for the course,” says Kipping. “Perhaps we’re not as unusual as some have speculated.”
Journal reference

Science

Jodrell Bank with Lovell telescope

Mysteries of the universe: Cheshire, England

Spend a weekend with some of the brightest minds in science, as you explore the mysteries of the universe in an exciting programme that includes an excursion to see the iconic Lovell Telescope.

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Chance of a devastating asteroid impact briefly spiked in 2025 /article/2502472-chance-of-a-devastating-asteroid-impact-briefly-spiked-in-2025/?utm_campaign=RSS|NSNS&utm_content=asteroids&utm_medium=RSS&utm_source=NSNS Wed, 10 Dec 2025 18:00:06 +0000 /?post_type=article&p=2502472 2502472