Decay of a Martian dust storm

The dust appears to be confined to the canyons, which can be as much as 8 km deep and hundreds of km wide.


Steve Lee (Univ. Colorado), Phil James (Univ. Toledo), and Mike Wolff (Univ. Toledo), and NASA/ESA

About the Image

NASA press release
Release date:15 July 1997, 19:00
Size:201 x 201 px

About the Object

Type:Solar System : Planet : Feature : Atmosphere
Category:Solar System

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16.6 KB
Screensize JPEG
85.1 KB

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