Ring mold crater

Ring Mold Craters are kind of crater on the planet Mars, that look like the ring molds used in baking. They are believed to be caused by an impact into ice. The ice is covered by a layer of debris. They are found in parts of Mars that have buried ice. Laboratory experiments confirm that impacts into ice result in a "ring mold shape." They are also bigger than other craters in which an asteroid impacted solid rock. Impacts into ice warm the ice and cause it to flow into the ring mold shape. These craters are common in Lobate Debris Aprons and lineated valley fill. Many have been found in Mamers Valles, a channel found along the dichotomy boundary in Deuteronilus Mensae.^[1][2][3] They may be an easy way for future colonists of Mars to find water ice.

• CTX context image for next image taken with HiRISE. Box indicates image footprint of following image.

• Possible ring mold crater, as seen by HiRISE under the HiWish program. Crater shape is due to impact into ice.

• Ring-mold craters form when an impact goes through to an ice layer. The rebound forms the ring-mold shape, and then dust and debris settle on the top to insulate the ice.

References

See also

• Lobate debris apron
• Concentric crater fill
• Glacier
• Deuteronilus Mensae