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

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