New Moon Crater Detected: A Rare Find | NASA's Lunar Reconnaissance Orbiter
This view from the side (55 degrees away from straight down) towards the east, covers an area of the Moon that is about 1.5 miles wide. It was taken by NASA's Lunar Reconnaissance Orbiter's Narrow Angle Camera (NAC) on March 3, 2026.
This view from the side (55 degrees away from straight down) towards the east, covers an area of the Moon that is about 1.5 miles wide. It was taken by NASA's Lunar Reconnaissance Orbiter's Narrow Angle Camera (NAC) on March 3, 2026.
An overhead, close-up view of McGetchin crater that was taken on Dec. 5, 2025, by NASA's Lunar Reconnaissance Orbiter (LRO) Narrow Angle Camera (NAC).
A zoomed-in view of McGetchin crater, circled on the left, next to a “before” image on the right. The panel on the left is made from images captured by NASA’s Lunar Reconnaissance Orbiter Wide-Angle Camera in summer 2025; the right panel was made from images taken in spring 2011. The white spot is not the crater itself, but rather material flung out of the crater. This formed when a rock, possibly this size of a three- to six‑story building, crashed into the Moon between April 11 and May 22, 2024—a once-in-a-century event, as scientists reported on Sept. 15, 2026, in a pair of papers in Science Advances. The area shown in these two images is 38 miles wide.
It started as a routine data-quality check. However, as Robert Wagner, a scientist with NASA’s Lunar Reconnaissance Orbiter (LRO), scanned a giant Moon map on his computer screen, an unusually large bright spot circled by a dark halo caught his eye, as it implied that surface material in that area had been shaken up.
“I just stopped, dropped everything, and started looking into what that spot was,” said Wagner, an image-processing specialist from Intuitive Machines that works with data from the Lunar Reconnaissance Orbiter Camera (LROC) system.
By comparing before and after images of the Moon, Wagner realized he had discovered the largest, newly formed crater ever found in the solar system, as scientists reported on Wednesday, Sept. 16, 2026, in Science Advances. This discovery highlights the value of NASA’s Moon orbiter data in studying a dynamic landscape as the agency advances a sustained human presence and expanded scientific and commercial activity on the Moon.
Officially named McGetchin after pioneering lunar scientist Tom McGetchin, the crater formed on the Moon’s eastern edge sometime between April 11 and May 22, 2024, after a comet or asteroid the size of a three- to six-story building hit the surface.
The crash left a crater, 728 feet wide, that spans the length of two football fields. And at 141 feet deep, the crater could fit three vertically stacked yellow school buses.
Scientists estimate that an impact of this magnitude happens on the Moon about once in a century or even longer.
The Moon takes hits
For more than 17 years, LRO has been circling the Moon and using its seven instruments to map the topography, surface composition, temperature, and radiation environment there. The spacecraft’s team has identified at least 1,000 new impact craters throughout the mission and flagged 100,000 more surface changes from an object smashing into the Moon or from the debris that flung out after.
With no atmosphere to slow them or burn them up, space rocks and other objects easily reach the lunar surface. Most are much smaller compared to the object that carved out McGetchin crater. The smallest craters scientists can distinguish from LRO images are about 30 feet wide, the length of a three-story building laid on its side, made by rocks about 43 inches wide, the size of a monster-truck tire. Scientists estimate that impacts of this scale produce about 140 new craters across the Moon each year. Nonetheless, most new ones are made by microscopic projectiles that leave holes too small to identify in orbital images.
With its numerous instruments, the spacecraft can observe changes to the lunar surface that are not apparent in the LROC images alone. After the crater was discovered, scientists working with LRO’s thermal instrument, Diviner, made follow-up observations of the site. They found a 4-mile-wide area around the crater that is about 16 degrees Fahrenheit cooler at night than its surroundings.
Reporting in a second paper Wednesday in the same journal, researchers say that the cooling happens because the impact fluffs up the regolith around the crater, making it less dense and therefore less able to retain heat.e
The large extent of this “cold spot” is striking, scientists say, because it shows that impacts can modify the Moon’s surface far beyond the crater itself. These physical changes could affect how rover wheels interact with the surface, for instance.
Road to discovery
The LROC system collects images from about 60 miles above the Moon as LRO loops from pole to pole. The system includes two cameras that capture high‑resolution black‑and‑white images and one camera for moderate‑resolution multispectral images. Over the years and thousands of passes, scientists have built maps detailed enough to spot not only new craters, but also landslides, landers, seismic faults, and even hints of lava tubes.
LROC scientists regularly analyze close-up images of small portions of the Moon's surface taken by the Narrow-Angle Camera. Using these images, they look for changes that are typically less than 30 feet across. Plus, every few years the team searches for large (wider than 150 feet) features by creating global Moon maps and comparing them to older versions.
This is what Wagner was doing on Oct. 24, 2025, when he came across McGetchin. Using images from LROC’s Wide-Angle Camera that captures broad views with pixels the size of football fields, he stacked hundreds of “before” and “after” frames with software designed to highlight change. Anything that stayed the same turned gray while anything different showed up as bright or dark patches.
While the process sounds straightforward, spotting real craters requires a lot of manual work. The software flags every tiny shift in lighting or shadow, generating hundreds of false alarms. For this reason, Wagner typically verifies the software, looking for small fuzzy halos around pixel‑wide bright points, which indicate splashes of regolith around a new crater.
Spanning hundreds of pixels, McGetchin stood out immediately. “It was by far the most obvious impact debris pattern I’ve ever seen in one of these images,” Wagner said.
After his discovery, scientists turned to the Narrow-Angle Camera, which takes much sharper views at about 3 feet per pixel. This camera’s close-up images, taken as LRO flew over the impact site again, revealed the crater size, shape, and how the surrounding terrain was affected. These images also helped researchers estimate the size and force of the rock fragment that formed the new crater, details that are expected to appear in a future paper.
NASA's Lunar Reconnaissance Orbiter has made a 3-D map of the Moon's surface at 100-meter resolution and 98.2% coverage (excluding polar areas in deep shadow), including 0.5-meter resolution images of Apollo landing sites.
LRO has been studying the Moon from up close since 2009, making it the longest-lived lunar orbiting mission ever. The orbiter has mapped the Moon’s surface and measured its temperature, composition, and radiation environment in unprecedented detail. Data from LRO enables NASA, and our international and commercial partners, to select locations on the lunar surface where spacecraft and astronauts can safely land. The orbiter is also helping NASA identify areas near the Moon’s South Pole with crucial resources like water and extended sunlight that provides power for equipment and supports exploration activities.
McGetchin lies one degree north of the lunar equator in the eastern hemisphere on the near side of the Moon. It sits at the boundary between volcanic mare basalt and ancient anorthosite highlands, near the outer rim of Crisium basin and 330 km (210 mi) from Mare Crisium. It measures on average 222 m (728 ft) in diameter and is up to 43 m (141 ft) deep. It is slightly asymmetrical, with a long axis of 231 m (758 ft) and a short axis of 213 m (699 ft). Its crater wall has slopes averaging 24°, reaching nearly 40° in some sections. The rim has an average height of 8 m (26 ft) above the pre-existing terrain.
Image Credits: NASA Goddard/Intuitive Machines/Robert Wagner
Article Credit: Lonnie Shekhtman
Release Date: March 8, 2018
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