Media Information

 
 
 
Collection:
NASA Solarsystem Collection
title:
Rampart Crater
description:
The ejecta deposits around Mars' impact crater Yuty (18 kilometers in diameter) consist of many overlapping lobes. Craters with this type of ejecta deposit are known as rampart craters. This type of ejecta morphology is characteristic of many craters at equatorial and midlatitudes on Mars, but is unlike that seen around small craters on the Moon. This style of ejecta deposit is believed to form when an impacting object rapidly melts ice in the subsurface. The presence of liquid water in the ejected material allows it to flow along the surface, giving the ejecta blanket its characteristic, fluidized appearance.

This image was taken in 1977 by the Viking 1 orbiter.

*Image Credit*: NASA
keywords:
Solar System Exploration
keywords:
SSE
keywords:
Space
keywords:
NASA
keywords:
National Aeronautics and Space Administration
keywords:
JPL
keywords:
Jet Propulsion Laboratory
keywords:
Planets
facet_what:
Mars
facet_what:
Crater
facet_what:
Moon
facet_what:
Viking
facet_what:
Viking 1 Orbiter
facet_where:
Jet Propulsion Laboratory
facet_where:
Mars
facet_where:
Jet Propulsion Laboratory (JPL)
facet_when:
1977
facet_when_year:
1977
UID:
SPD-SLRSY-824
original url:

Rampart Crater