Impact crater

Kepler

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

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Kepler and surrounding lunar terrain in the LROC Wide Angle Camera mosaic
Kepler · 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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How to observe Kepler

Use higher illumination to trace the rays over the darker plains, then revisit near the terminator for the crater itself.

Finding the region

Look at 8.12° N, 38.01° 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 Kepler in the atlas →

IAU / USGS Gazetteer

Official feature record

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Approved name
Kepler
Feature classification
Crater, craters
Catalogue diameter
29.49 km
Centre latitude
8.12° N
Centre longitude
38.01° W
Name origin (Gazetteer)
Johannes; German astronomer (1571-1630).

Selenographic coordinates · East-positive longitude · Catalogue extent · Updated 2026-09-16

Nearby formations

LROC photograph of CopernicusImpact crater

Copernicus

A prominent impact crater south of Mare Imbrium. It has terraced inner walls, central peaks and a broad field of ejecta.

LROC photograph of AristarchusImpact crater

Aristarchus

A bright crater beside the darker Aristarchus plateau in Oceanus Procellarum. Vallis Schroteri winds across the neighbouring plateau.

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 Vallis SchroteriValley / rille / scarp

Vallis Schroteri

A winding valley on the Aristarchus plateau. Its shape contrasts with the straight fractures and impact features elsewhere on the Moon.