In the spring of 2024, a fragment of an asteroid or comet slammed into the Moon, unleashing a violent eruption of shattered rock and lunar dust that carved the 222-meter-wide McGetchin crater. No one witnessed the collision, and its extraordinary aftermath remained undiscovered until NASA’s Lunar Reconnaissance Orbiter revealed the evidence more than a year later. AI-generated artistic interpretation.

12 / The Moon / three different measures of reach

The Lunar Impact Whose Footprint Outgrew Its Crater

McGetchin crater is 222 meters across, yet orbital image comparisons found localized surface disturbances about 140 kilometers away. The visible hole, thermal cold spot and distant optical changes measure different consequences of one impact.

The Moon records changes without an atmosphere to carry ordinary weather across them. When fresh orbital images reveal a crater absent from an earlier frame, the interval constrains its formation and the surrounding terrain becomes a before-and-after experiment. McGetchin formed between April and May 2024 and was recognized later in the image record. Its scattered optical changes and altered nighttime temperatures show that an impact can modify regolith beyond the obvious excavation. The correct scale depends on which instrument and which kind of modification is being described.

The full investigation continues with the evidence, illustrations, and sources at The Last Transmission on Substack.

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THE EVIDENCE / THE OPEN QUESTION

01 / THE OBSERVATION

What we know.

NASA reports a crater about 222 meters wide and approximately 43 meters deep. The research distinguishes a thermal cold spot around seven kilometers in diameter from localized distal optical disturbances extending to roughly 140 kilometers radially. These observations describe surface and thermal properties; they are not interchangeable measurements of a single destructive blast zone.

02 / THE UNKNOWN

What remains open.

The distant detections do not establish uniform devastation across a 140-kilometer circle, a 140-kilometer-deep fracture, or a measured lethal radius for astronauts. Regolith structure, ejecta and related surface processes need to be separated when explaining the changed brightness and heat retention. A cold spot is not evidence of discovered lunar ice.

03 / THE BIGGER PICTURE

Why it matters.

Impact planning has to account for more than the size of the final hole. Before-and-after imaging and thermal measurements reveal processes that static crater counts can miss. Translating those measurements into engineering risk will require modeling and validation appropriate to actual habitats and equipment, rather than treating a striking distance as a ready-made safety boundary.

FOLLOW THE EVIDENCE

Research behind the field note.

A 222-m diameter lunar crater Lunar crater reveals extensive distal regolith modification NASA research-team account, 2026-09-16 Deep Structure of the Lunar South Pole–Aitken Basin

VISUAL EVIDENCE

Inside the investigation.

Visual archive
In the spring of 2024, a fragment of an asteroid or comet slammed into the Moon, unleashing a violent eruption of shattered rock and lunar dust that carved the 222-meter-wide McGetchin crater. No one witnessed the collision, and its extraordinary aftermath remained undiscovered until NASA’s Lunar Reconnaissance Orbiter revealed the evidence more than a year later. AI-generated artistic interpretation.
In the spring of 2024, a fragment of an asteroid or comet slammed into the Moon, unleashing a violent eruption of shattered rock and lunar dust that carved the 222-meter-wide McGetchin crater. No one witnessed the collision, and its extraordinary aftermath remained undiscovered until NASA’s Lunar Reconnaissance Orbiter revealed the evidence more than a year later. AI-generated artistic interpretation.
Long after the violence of the initial collision, its effects continued to reshape the lunar surface. The impact scattered rock and disturbed ancient layers of powder-fine regolith, leaving subtle changes in the Moon’s surface texture that extended more than 100 kilometers from the crater, revealing how a single moment of destruction can alter a landscape far beyond the visible scar. AI-generated artistic interpretation.
Long after the violence of the initial collision, its effects continued to reshape the lunar surface. The impact scattered rock and disturbed ancient layers of powder-fine regolith, leaving subtle changes in the Moon’s surface texture that extended more than 100 kilometers from the crater, revealing how a single moment of destruction can alter a landscape far beyond the visible scar. AI-generated artistic interpretation.
An imagined ancient lunar-basin landscape evokes the South Pole–Aitken question. Gravity measurements support excess mass at depth; this surface artwork does not show the buried mass or identify its composition. AI-generated conceptual illustration.
An imagined ancient lunar-basin landscape evokes the South Pole–Aitken question. Gravity measurements support excess mass at depth; this surface artwork does not show the buried mass or identify its composition. AI-generated conceptual illustration.

FOLLOW THE THREAD

Related signals.

THE SIGNAL CONTINUES

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