Low temperature aqueous ferric sulfate solutions on the surface of Mars

Physics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

35

Planetary Sciences: Solar System Objects: Mars, Geochemistry: Geochemical Modeling (3610, 8410), Geochemistry: Thermodynamics (0766, 3611, 8411), Global Change: Geomorphology And Weathering (0790, 1824, 1825, 1826, 1886)

Scientific paper

We have studied the low-temperature properties of ferric sulfate Fe2(SO4)3 solutions as a model for potential liquid brines on the surface of Mars. Geochemical modeling demonstrates that concentrated ferric sulfate brines form through sulphur-rich acidic evaporation processes in cold oxidizing environments. Experiments and thermodynamic calculations show that the Fe2(SO4)3 eutectic temperature is 205 +/- 1 K for 48 +/- 2 wt% concentration. As a result of low water activity, these solutions exhibit evaporation rates ranging from 0.42 mm h-1 (29.1 wt%) to 0.03 mm h-1 (58.2 wt%), thus down to 20 times lower than pure water. The combination of extremely low eutectic temperature and evaporation rates allow subsurface liquids to be stable at high latitudes, where the majority of gullies and viscous flow features are located. Therefore, we conclude that episodic releases of highly concentrated ferric sulfate brines are a potential agent for the formation of recent and present-day gullies on Mars.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Low temperature aqueous ferric sulfate solutions on the surface of Mars does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Low temperature aqueous ferric sulfate solutions on the surface of Mars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Low temperature aqueous ferric sulfate solutions on the surface of Mars will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-747312

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.