Anonymous user
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)
Revision as of 05:44, 28 September 2018
, 5 years ago→Southern hemisphere flow-like features
No edit summary |
|||
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 [[Richardson (Martian crater)|Richardson Crater]] in the Martian southern hemisphere- one of the places where the Flow Like Features (FLFs) have been observed.
Line 89 ⟶ 84:
For details see the Dark Dune Spots section of Nilton Renno's paper<ref name="MartínezRenno2013DarkDuneSpots"/> which also has images of the two types of feature as they progress through the season.
==Earlier hypotheses==
|