Potentially habitable flow-like features from Martian dry ice geyser dune spots: Difference between revisions

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==Southern hemisphere flow-like features==
The process starts with the dark dune spots which form in early spring. Here are some examples in [[{{Wikipedia|Richardson (Martian crater)|Richardson Crater]]}} in the Martian southern hemisphere- one of the places where the Flow Like Features (FLFs) have been observed.
 
{{Wide image |WikirichardsonPSP_002885_1080.jpg|800px|Dark dune spots in Richardson crater}}
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