USGS

Venus Crater Database

Catagories Included in the Database



Crater Type

Larger versions of most sample images are available by selecting either the modification class, the thumbnail image or crater name. The size of the larger image is given in kilobytes (kb). Large images are all at a scale of 225 m/pixel. They have not been stretched to enhance contrast, but retain the full radiometric calibration [Pettengill and others, 1991].

The types of crater morphologies listed on the data base are as follows:

Mona Lisa B, multi-ring basin--large crater containing more than one concentric ring of low ridges or hills protruding above the floor inside the crater's dominant rim.
Mona Lisa (79 km in diameter; 25.61°N, 25.15°E). (1 mb)

Cochran D, double-ring basin--large crater containing only a single concentric ring inside the crater rim.
Cochran (100 km in diameter; 51.86°N, 143.36°E). (2.15 mb)

Saskia P, central peak--crater containing a single peak or closely grouped cluster of peaks or hills that is more or less centered on and rises above the crater floor deposits.
Saskia (37 km in diameter; 28.58°S, 337.12°E). (220 kb)

Sabira S, structureless floor--crater containing no recognizable structures on the crater floor; crater floor sometimes flooded with impact-generated lava from below, or (rarely) a local volcanic source.
Sabira (15.7 km in diameter; 5.75°S, 239.86°E). (40 kb)

Lotta I,P, irregular(I) with central peak(P)--crater characterized by an generally non-circular (irregular) rim and hummocky wall and floor deposits; thought to result from a cluster of parent asteroid or cometary material disrupted and slowed down by the venusian atmosphere prior to impact.
Lotta (12 km in diameter; 51.06°N, 335.91°E). (40 kb)

image M, multiple--impact crater, thought to result from the impact of a parent asteroid or cometary nucleus that was totally disrupted and whose fragments were dispersed low in the atmosphere into separate individual trajectories just prior to impact. [Note: diameters given for multiple craters is associated with the largest crater within the crater group, and not for the diameter of the entire group of craters.]
Terhi; multiple crater; largest crater in field, 10.7 km in diameter; total size of field 30X52 km (45.71°N, 253.09°E). (156 kb)


Title Page Table of Contents Introduction The Crater Database Download
the Database
General Information References
Categories Included in the Database
Names Modification State Crater Type Elevation