Impact crater

Grimaldi

A conspicuously dark enclosed plain near the western limb. Its strong contrast makes it a useful landmark even when fine relief is difficult to see.

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Grimaldi and surrounding lunar terrain in the LROC Wide Angle Camera mosaic
Grimaldi · North up, east right. Open image ↗
NASA / GSFC / Arizona State University · LROC WAC mosaic via USGS. Regional map crop; lighting is fixed and does not follow the selected date.
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Lunar north up, with geocentric libration. Full atlas mode shows the entire facing surface; switch to Selected phase for today’s illumination. Choose a different date in the atlas.

How to observe Grimaldi

Compare the dark interior with the adjacent highlands. Check how libration changes its apparent width.

Finding the region

Look at 5.38° S, 68.36° W on the lunar disc. The chart marker identifies the catalogue centre. Start with a wide field and use the nearby formations below as landmarks.

Equipment & conditions

Start at low magnification to identify the rim. Move to a moderate power when the air is steady; low sunlight usually makes walls and floor relief easier to distinguish. A bright ray system can be more conspicuous near full Moon.

Lighting

For surface relief, try a time when the Sun is low over this region. To compare surface brightness and any bright rays, return under higher illumination. The atlas calculates the solar elevation at the formation’s centre for any selected date.

View Grimaldi in the atlas

IAU / USGS Gazetteer

Official feature record

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Approved name
Grimaldi
Feature classification
Crater, craters
Catalogue diameter
235.00 km
Centre latitude
5.38° S
Centre longitude
68.36° W
Name origin (Gazetteer)
Francesco Maria; Italian astronomer, physicist (1618-1663).

Coordinates are selenographic, with east-positive longitude. Dimensions are the Gazetteer’s catalogue values; for extended formations they do not represent a circular crater diameter. Data snapshot: 2026-09-16. Observing guidance above is separate from the official record.

Nearby formations

The four closest catalogue entries, measured from their centres.

LROC photograph of Oceanus ProcellarumSea / bay

Oceanus Procellarum

The Ocean of Storms is an extensive dark region across the western near side. Unlike the compact circular maria, it has a broad irregular outline.

2,592.2 kmRead guide ↗
LROC photograph of GassendiImpact crater

Gassendi

A large crater on the northern edge of Mare Humorum. Its floor contains central peaks and a network of fractures.

LROC photograph of KeplerImpact crater

Kepler

An isolated ray crater in the western maria, smaller than Copernicus but easy to locate by its bright surroundings.

LROC photograph of Mare HumorumSea / bay

Mare Humorum

The Sea of Moisture is a rounded dark plain in the southwestern near side. Gassendi marks its northern edge.