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About: Dark slope streak     Goto   Sponge   NotDistinct   Permalink

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Type: yago:WikicatSurfaceFeaturesOfMarsyago:Abstraction100002137yago:Cognition100023271yago:Concept105835747yago:Content105809192yago:Feature105849789yago:Idea105833840yago:Property105849040yago:PsychologicalFeature100023100building New Facet based on Instances of this Class

Dark slope streaks are narrow, avalanche-like features common on dust-covered slopes in the equatorial regions of Mars. They form in relatively steep terrain, such as along escarpments and crater walls. Although first recognized in Viking Orbiter images from the late 1970s, dark slope streaks were not studied in detail until higher-resolution images from the Mars Global Surveyor (MGS) and Mars Reconnaissance Orbiter (MRO) spacecraft became available in the late 1990s and 2000s.