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

Potentially habitable flow-like features from Martian dry ice geyser dune spots (edit)

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Revision as of 05:44, 28 September 2018 (edit) 213.122.219.3 (talk) (→‎Southern hemisphere flow-like features) ← Older edit		Revision as of 05:46, 28 September 2018 (edit) (undo) 213.122.219.3 (talk) (→‎Southern hemisphere flow-like features) Newer edit →
Line 15: __TOC__ ==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}}