NASA‘s LRO (Lunar Reconnaissance Orbiter) has captured and released the first confirmed images of the Falcon 9 crater a SpaceX rocket stage carved into the Moon. The pictures did more than confirm the impact happened. They revealed exactly how big the scar is, what it’s made of, and how difficult it was to photograph at all.
Between Aug. 11 and 12, LRO’s cameras caught the fresh crater near Einstein crater on the Moon’s western near side. NASA published the imagery and analysis on Aug. 18. The crater formed Aug. 5. The spent upper stage was leftover hardware from a January 2025 launch that sent Firefly Aerospace’s Blue Ghost 1 lander toward the Moon. It slammed into the surface after nearly 19 months adrift in an uncontrolled orbit.
FODNews reported the impact itself on Aug. 7, when the only evidence was a telescope-detected plume of vaporized sodium and lithium. The new LRO images of the Falcon 9 crater are the first direct, visual confirmation. They answer questions the earlier spectroscopy couldn’t.
LRO images refine the Falcon 9 crater’s true size
Pre-impact models had estimated a crater somewhere between 20 and 30 meters (65 to 90 feet) wide. The actual LRO measurements came in smaller. The crater measures about 60 feet (18 meters) across, measured from the rim under favorable lighting. It’s also less than 10 feet deep, estimated from the length of the crater’s shadow.
Capturing that detail required LRO’s Narrow-Angle Camera, which resolves surface features as small as 3 feet wide. The imagery also caught the crater under multiple lighting angles as LRO’s orbit shifted. That let scientists pick out details a single pass would have missed.
Bright and dark ejecta rays expose a cross-section of the Moon
The most scientifically useful part of the images may be the ejecta pattern radiating from the crater. Dark streaks fan out from weathered lunar regolith excavated from about 1.5 feet below the surface. That material spent eons exposed to solar wind, cosmic rays and micrometeorite bombardment. Brighter streaks closer to the rim come from fresh material blasted up from deeper underground. It hasn’t yet been darkened by space weathering.
Together, the two ray types give researchers a natural cross-section of the lunar subsurface. A four-ton piece of space hardware, traveling roughly 5,400 mph, generated it instantly.
A six-day wait and a 10-second margin
Getting the shot was its own story. LRO orbits the Moon pole-to-pole every two hours. It moves at roughly 1 mile per second at an altitude of about 60 miles. To photograph a specific spot, engineers had to tilt the spacecraft’s cameras toward the crater on each pass. Then they had to wait for the Moon’s slow rotation to carry the target into view. It took six days before the ground track finally lined up.
Timing had almost no room for error. NASA said a camera trigger off by just 10 seconds would have drifted the target 10 miles out of frame. That would have wasted the pass entirely.
Amateur trackers, CNEOS and Korea’s Danuri all played a role
The imaging campaign only worked because of tracking coordination that started well before LRO ever tilted its cameras. Independent astronomers first identified the doomed rocket stage’s trajectory using publicly available tracking data. NASA’s Center for Near Earth Object Studies (CNEOS) at the Jet Propulsion Laboratory normally tracks natural objects that threaten Earth for NASA’s planetary defense program. This time, CNEOS used the opportunity to test and validate its own impact-prediction tools on a real, non-hazardous event.
CNEOS incrementally refined its impact-location estimate and passed coordinates to Danuri, the Republic of Korea’s Korea Pathfinder Lunar Orbiter. Danuri’s high-resolution LUTI camera imaged the crater first, on Aug. 5-6. It found CNEOS’s prediction accurate to within about 0.6 miles. Danuri then sent its own coordinates back to NASA. That helped the LRO team refine its follow-up imaging sequence. It ultimately pinned down updated crater coordinates: 19.4759°N, 266.7138°E, at 511 meters elevation.
Why it matters for debris tracking
The Falcon 9 crater episode is a real-world test of the tracking pipeline used to predict where uncontrolled objects will come down. It’s technology with direct relevance to orbital debris and reentry risk here at Earth. A trajectory identified by amateur observers got refined by a planetary-defense team built to watch for hazardous asteroids. An international partner orbiter then cross-checked it, confirming sub-mile accuracy. That’s exactly the kind of coordination NASA and other agencies will need. More derelict rocket stages and defunct satellites will end up on uncontrolled trajectories, whether toward the Moon or back toward Earth.
It’s also a reminder that lunar-transfer trajectories don’t guarantee a clean exit from the Earth-Moon system. Upper stages with no propellant left for a disposal burn can drift for years. Gravity and solar radiation pressure eventually decide where they land.
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Sources
- NASA Science. “NASA’s LRO Images Falcon 9 Crater on Moon, Learns New Details.”
- CNN. “NASA images show crater left by SpaceX rocket that hit the moon” (Aug. 18, 2026).
- Le Monde. “NASA images show crater on Moon left by SpaceX rocket” (Aug. 19, 2026).
- The Register. “NASA estimates the size of the hole SpaceX made in the Moon” (Aug. 19, 2026).
- FODNews. “SpaceX Booster Hit the Moon at 5,400 MPH” (Aug. 7, 2026).
