Illustration accompanying What Does a 140-Kilometer Lunar Disturbance Actually Mean?

EVIDENCE FILE 21 / LUNAR IMPACTS

What Does a 140-Kilometer Lunar Disturbance Actually Mean?

How do a crater, a thermal cold spot and localized optical changes give three different measures of an impact?

All Evidence Files
By The Last TransmissionResearch reviewed October 16, 2026Original research explainer

THE SHORT ANSWER

Orbital comparisons reveal more than the excavated hole. The approximately 140-kilometer figure describes the radial reach of localized subtle optical disturbances, while the smaller thermal cold spot and crater measure different effects. It is not a uniform destruction radius.

THE EVIDENCE MAP / LUNAR IMPACTS

How do a crater, a thermal cold spot and localized optical changes give three different measures of an impact?

Separate McGetchin’s 222-meter crater, approximately seven-kilometer cold-spot diameter and localized optical effects roughly 140 kilometers away.

  1. 01Measurement

    Compare orbital images and thermal measurements

    Before-and-after imagery brackets the event and locates optical changes. Thermal observations characterize altered nighttime behavior, adding another kind of evidence about the regolith.

  2. 02Interpretation

    Assign each scale to the property measured

    Crater diameter, cold-spot diameter and distal optical reach are three different quantities. Their numbers become meaningful only when the observed property and radial or diameter convention remain explicit.

  3. 03Competing explanation

    Distinguish patchy change from a blast boundary

    Localized remote changes do not show that all intervening terrain experienced the same disturbance. Ejecta and regolith mechanisms need models that reproduce the actual distribution.

  4. 04Open test

    Validate models relevant to lunar infrastructure

    Future comparisons should connect measured terrain modification with physical transport and equipment response. A habitat safety criterion needs that additional engineering evidence.

TRACE THE CLAIM / THEN TEST ITResearch: A 222-m diameter lunar crater Lunar crater reveals extensive distal regolith modification

OBSERVATION / INFERENCE / LIMIT

Read the signal.

THE HOLE

222 meters across

the impact crater is about 43 meters deep; these are excavation dimensions, not the extent of every effect.

THERMAL CHANGE

About 7 km diameter

The nighttime cold spot concerns altered heat retention around the crater, rather than discovered ice.

DISTAL SIGNAL

Up to roughly 140 km

Localized optical/regolith disturbances reach far from the impact; the figure is radial and does not imply uniform damage.

INSIDE THE EVIDENCE

The chain of reasoning.

Each step has a different level of certainty. Follow the measured result into the explanation, then see where the trail ends.

01 / LUNAR IMPACTS

A before-and-after pair establishes an event

Lunar Reconnaissance Orbiter images show a crater absent from an earlier observation and present in a later one. That comparison brackets its formation between April and May 2024, while its later recognition reflects the time required to identify the change in the archive. The approximately 222-meter diameter and 43-meter depth characterize the excavation. They give a starting point for studying the event, but the surrounding surface can preserve effects that require different kinds of observations to recognize.

02 / LUNAR IMPACTS

Optical changes need their own spatial description

A changed appearance in orbital images can reflect disturbed regolith, ejecta or other modifications of surface texture and reflectance. The research distinguishes more continuous nearby changes from localized effects detected at much greater distance. The roughly 140-kilometer figure describes that distant radial reach. It should not be redrawn as a uniformly altered disk simply because a circle makes a striking graphic. The distribution, detectability and physical cause of each changed patch matter when interpreting the optical measurement.

03 / LUNAR IMPACTS

Thermal observations ask a different question

Nighttime temperature depends on how the upper surface stores and releases heat. A thermal cold spot can therefore reveal regolith modification that is not identical to the brightest optical ejecta. The reported maximum cold-spot extent is about seven kilometers in diameter, a separate scale from the approximately 140-kilometer optical reach. Cooler nighttime measurements do not establish frozen water. They motivate a physical account of altered thermal properties and surface structure under the observed illumination and timing.

04 / LUNAR IMPACTS

Separate mechanism from measured change

An impact can distribute material and disturb surface layers in several ways. Image differences and thermal signatures constrain what changed without independently deciding the contribution of every proposed mechanism. Matching a physical model requires accounting for the pattern and scale of the observations together. A cinematic eruption makes the event imaginable, but its glowing debris and camera position are invented. The orbital record, rather than an artist’s blast, is what supports the claim of a much broader footprint than the final hole.

05 / LUNAR IMPACTS

Engineering risk requires a further translation

These observations are relevant to lunar infrastructure because a distant impact may affect more terrain than crater dimensions alone suggest. The next step is a validated relationship among impact conditions, ejecta, local disturbances and the vulnerabilities of actual equipment. The study does not by itself establish a lethal radius for astronauts or a universal safe distance for habitats. Keeping that distinction visible allows the science to inform planning without converting a subtle measured surface change into an unsupported prediction of uniform destruction.

THE EASY MISREADING

The 140-kilometer reach is neither a 140-kilometer-wide crater nor a uniformly devastated area, and the thermal cold spot is not an ice discovery.

PRIMARY RESEARCH & MISSION RECORDS

Check the source.

These are the studies and mission records behind this explainer. The illustrated article and related research pages continue the investigation.

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

FOLLOW THE THREAD

Stay with the question.

Continue through the original Field Note, the complete illustrated article and the relevant explorer. Each route keeps the measurement distinct from the artistic reconstruction.

The Lunar Impact Whose Footprint Outgrew Its Crater

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