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Grand Canyons on the Moon Were Made in a Matter of Minutes

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Grand Canyons on the Moon Were Made in a Matter of Minutes

Two canyons near the south pole of the moon rival the Grand Canyon, both in depth and length.

Unlike the sinuous chasm in Arizona, the two lunar canyons, known as Vallis Schrödinger and Vallis Planck, are straight, as if the crust of the moon had been cut by a knife.

And unlike the Grand Canyon, carved over millions of years by the flow of the Colorado River, Vallis Schrödinger and Vallis Planck formed in just minutes after a 15-mile-wide meteor struck the moon some 3.8 billion years ago.

Indeed, carving these vast lunar trenches took less time than it might take you to bake a frozen pizza.

The impact, comparable to the one that smashed into the Earth 66 million years ago and killed the dinosaurs, punched up to 15 miles into the crust and excavated a crater about 200 miles wide. In the process, it ejected fusillades of giant rocks — what planetary scientists call ejecta rays — that crashed down in staccato succession to create the canyons, which are more than 1.5 miles deep and more than 165 miles long.

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“They truly are extraordinary in scale,” said David Kring, a scientist at the Lunar and Planetary Institute in Houston. “These things were carved in less than 10 minutes when the Grand Canyon took 5 to 6 million years to carve. I mean that illustrates the energy of an impact event.”

In a new analysis, Dr. Kring and his colleagues, Danielle Kallenborn and Gareth Collins of Imperial College London, constructed a mathematical model to describe how the canyons formed in a rain of giant rocks. They used photographs taken by NASA’s Lunar Reconnaissance Orbiter, which showed a string of craters along the canyons, to calculate the speed and direction of the debris.

“Imagine a kilometer- or a five-kilometer rock hitting the ground at over 2,000 miles per hour,” Dr. Kring said. “Each one of these blocks will produce a crater about 20 kilometers in diameter. And they hit the ground — bang, bang, bang, bang, bang.”

The scientists calculated that the energy needed to create the two canyons was more than 130 times what would be produced in an explosion of all the nuclear weapons that exist on Earth today.

Their findings appear in a paper published on Tuesday in the journal Nature Communications.

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The canyons also suggest that the incoming asteroid or comet hit at an angle even though the crater itself is almost circular in shape.

The straight lines of Vallis Schrödinger and Vallis Planck radiate outward from the Schrödinger basin crater. But the scientists noticed that the lines, if extended, did not intersect at the center of the crater.

Instead, the intersection point is to the south. That is likely where the space rock hit, the scientists said.

“I think they’ve got the interpretation right on that,” said Jennifer Anderson, a professor of geoscience at Winona State University in Minnesota. “These ginormous crater rays, they point back to a point that is up range of the center of the crater.”

That indicates that the meteor came from the south and that the curtain of debris was largely kicked to the north, away from the south pole.

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That is an encouraging finding for Artemis, NASA’s return-to-the-moon program, because it suggests that the areas near the south pole where the agency wants to land astronauts are not covered by debris from the Schrödinger impact and that rocks from a much larger, much older impact known as the South Pole–Aitken basin would be exposed at the surface.

Dr. Anderson said the new findings matched with small-scale laboratory experiments she had conducted a couple of decades ago, firing BB-size pellets into sand, which created craters less than a foot in diameter.

“It’s the farthest ejecta on the surface that tell you about what happened at earliest times in the cratering event,” she said.

What is less certain is how the impact produced a long, narrow stream of rocks in the ejecta rays instead of a more uniform cascade in all directions.

“We still debate the origin,” Dr. Kring said.

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The ejecta rays might have resulted from earlier craters or other unevenness of the terrain. “It could have been two preexisting craters caused the focusing of some of this debris into these rays,” Dr. Kring said.

Dr. Anderson said such rays also occurred in her small-scale experiments, and she, too, could not explain that phenomenon.

“We can see that there are areas of the ejecta curtain that are more dense with material as opposed to less dense,” she said. “Why that is, I don’t know that anyone knows yet, except that nature is messy.”

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Video: SpaceX Launches NASA’s Crew-10 Mission

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Video: SpaceX Launches NASA’s Crew-10 Mission

new video loaded: SpaceX Launches NASA’s Crew-10 Mission

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SpaceX Launches NASA’s Crew-10 Mission

The mission would allow Suni Williams and Butch Wilmore, two NASA astronauts, to return to Earth. Their brief scheduled visit to the space station last June was unexpectedly stretched to more than nine months.

“Ignition and liftoff.” [cheering] “[unclear] and liftoff as Crew-10 now soaring to International Space Station.” “Great callouts and incredible views there on your left-hand screen. In your left-hand screen, you can see a view from Stage 1.” [cheering] “The first stage making its way back down to Earth, and the second stage continuing to fire.” [cheering] “There, on the right-hand side of your screen, you can see some first images of Crew-10 inside the Dragon Endurance spacecraft, as they’re now successfully in orbit.”

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Photos Show Blood Moon Lunar Eclipse Around the World

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Photos Show Blood Moon Lunar Eclipse Around the World

From Thursday night into Friday morning, the Earth’s shadow gradually overtook the moon’s typically bright white face, which took on a ruddy red hue. It was the first total lunar eclipse, also known as a blood moon, in more than two years.

A lunar eclipse occurs when the sun, Earth and moon align, in that order. There are different types of lunar eclipses, but total lunar eclipses cause the moon to shine red because sunlight must travel through the atmosphere before illuminating the moon. Blue wavelengths of light scatter more readily in our atmosphere, but redder wavelengths pass through, creating the blood-moon effect.

The blood moon was most visible this week in the Americas, western parts of Africa and Europe, New Zealand and some of Russia.

Local stargazing groups and planetariums in many cities hosted watch parties, while others got the chance to see it online. Totality, when the entire moon is engulfed in the darkest part of Earth’s shadow, was expected at 2:25 a.m. Eastern.

But anyone who missed it won’t have to wait long for another chance. Lunar eclipses can occur several times a year, though not all of them reach totality. According to NASA, the next total lunar eclipse will occur in September, most visible in Asia and parts of Europe, Africa and Australia. There will be another total lunar eclipse next March, followed by a partial lunar eclipse in August 2026.

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Humanity’s well-documented and ancient fascination with the Earth’s only natural satellite means that stargazers across the planet last night participated in an activity as old as time: They turned their eyes to the sky. Here’s what that looked like in different locations around the world:

Katrina Miller contributed reporting.

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Video Shows Mars and Deimos Close Up During ESA’s Hera Flyby

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Video Shows Mars and Deimos Close Up During ESA’s Hera Flyby

An asteroid-chasing spacecraft just swung past Mars on Wednesday. As it zipped by, it took hundreds of shots of the Red Planet, as well as several snaps of Deimos, one of the two small Martian moons.

The operators of the European Space Agency’s Hera spacecraft were bewitched by the sci-fi aesthetics of the pictures.

“We were waiting with impatience to get these images,” said Patrick Michel, the principal investigator for Hera, during a Thursday news conference at mission control in Darmstadt, Germany. When the first shots of the moon appeared, many of the Hera team members burst into cheers. “We’ve never seen Deimos in that way,” Dr. Michel said.

Navigators managed to fly Hera about 600 miles above Deimos, a craggy moon just nine miles long. The pass shows the object in remarkable detail — a small island gliding above the crater-scarred Martian desert.

During the news conference, Ian Carnelli, the Hera project manager, was misty-eyed. “I’m going to get emotional,” he said. “The excitement was such that we didn’t get any sleep.”

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Hera was using Mars in what is known as a gravity assist, both accelerating the spacecraft and adjusting its flight path. But its mission operators also wanted to take advantage of the Martian flyby and use it to test the mechanical eyes that will allow Hera to study the asteroid it is targeting, Dimorphos.

In the coming days, the mission’s scientists will reveal more photographs from Hera’s encounter with Mars, which may include shots of Phobos, the planet’s other moon.

As with any planetary flyby, there were some nerves about whether Hera would conduct its maneuvers properly and end up on the right trajectory. “The spacecraft behaved very well,” said Sylvain Lodiot, the Hera operations manager. “We’re on track to the asteroid system.”

Hera is headed to Dimorphos as a follow-up to a 2022 NASA mission, the Double Asteroid Redirection Test. DART deliberately crashed a spacecraft into that asteroid, aiming to change its orbit around a larger asteroid, Didymos. That was a test of whether a dangerous space rock bound for Earth could be deflected in a similar manner.

The experiment successfully changed the orbit of Dimorphos. But the asteroid’s physical nature, and its full response to DART’s collision, remains unclear; some evidence suggests that it acted like a fluid when hit, rather than a solid, causing it to eject a lot of debris and reshape itself.

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When it comes to stopping lethal asteroids from striking Earth, the more scientists know about their rocky enemies, the better prepared they will be should one come careening our way. To aid that effort, the European Hera mission will arrive at Dimorphos in late 2026 for a close-up study of the DART-impacted asteroid.

This Wednesday, during Hera’s flyby of Mars and Deimos, the spacecraft used three cameras — including a thermal infrared imager supplied by the Japan Aerospace Exploration Agency.

Mars’s two moons have mysterious origins. Both could be pieces of a disintegrating asteroid captured by the planet’s gravity, or perhaps the flotsam and jetsam leftover from a giant impact event on Mars.

Deimos is tidally locked, meaning one hemisphere permanently faces Mars. This near side is the one most commonly seen by spacecraft orbiting the planet, or by rovers driving across its surface. Hera managed to fly behind Deimos, meaning it caught a rare sight.

“It’s one of the very few images we have of the far side of Deimos,” said Stephan Ulamec, a researcher at the German Aerospace Center and member of the Hera team.

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This opportunistic peek at Mars and Deimos was exciting. But the team is especially thrilled that Hera is now on its way to its asteroid destination. “We’re all looking forward to what Didymos and Dimorphos will look like,” Dr. Michel said.

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