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Subsurface Cl-bearing salts as potential contributors to recurring slope lineae (RSL) on Mars
| Content Provider | Semantic Scholar |
|---|---|
| Author | Wang, Alian Ling, Zongcheng Yan, Yuanchao Mcewen, Alfred S. Mellon, Michael Tyler Smith, Michael D. Jolliff, Bradley L. Head, James W. Iii |
| Copyright Year | 2019 |
| Abstract | Abstract We report laboratory experimental results that support a brine-related hypothesis for the recurring slope lineae (RSL) on Mars in which the subsurface Cl-salts, i.e., hydrous chlorides and oxychlorine salts (HyCOS) are the potential source materials. Our experiments revealed that within the observed RSL temperature window T RSL (250–300 K), the deliquescence of HyCOS could occur in relative humidity ranges (RH ≥ 22%–46%) much lower than those for hydrous (Mg, Fe)-sulfates (RH ≥ 75%–96%). In addition, we demonstrated that the RH values kept by common HyCOS and hydrous sulfates in enclosures have a general trend as RH sulfates > RH perchlorates > RH chlorides (with same type of cation) in wide T range. It means that the required RH range for a Cl-bearing salt to deliquescence can be satisfied by a co-existing salt of different type, e.g., in the subsurface layers of mixed salts on Mars. Furthermore, we found a strong temperature dependence of the deliquescence rates for all tested HyCOS, e.g., a duration of 1–5 sols for all HyCOS at the high end (300 K) of T RSL , and of 20–70 sols for all tested HyCOS (except NaClO 4 ·H 2 O) at the low end (250 K) of T RSL , which is consistent with the observed seasonal behavior of RSL on Mars. From a mass-balance point of view, the currently observed evidences on Mars do not support a fully-brine-wetted track model , thus we suggest a brine-triggered granular-flow model for the most RSL. Considering the recurrence of RSL in consecutive martian years, our experimental results support the rehydration of remnant HyCOS layers during a martian cold season through H 2 O vapor-to-salt direct interaction. We found that the evidences of HyCOS rehydration under Mars relevant P-T-RH conditions are detectable in a few minutes by in situ Raman spectroscopy. This rehydration would facilitate the recharge of H 2 O back into subsurface HyCOS, which could serve as the source material to trigger RSL in a subsequent warm season. The major limiting factor for this rehydration is the H 2 O supply, i.e., the H 2 O vapor density carried by current Mars atmospheric circulation and the diffusion rate of H 2 O vapor into the salt-rich subsurface in a cold season. In a worst-case scenario, these H 2 O supplies can support a maximum increase of hydration degrees of two for totally dehydrated HyCOS, whereas the full rehydration of subsurface HyCOS layers can be easily reached during a >30° obliquity period that has H 2 O vapor density 10× to 20× times the value of current obliquity. Overall, our results imply the existence of a large amount of Cl-bearing salts in the subsurface at RSL sites. |
| Starting Page | 464 |
| Ending Page | 480 |
| Page Count | 17 |
| File Format | PDF HTM / HTML |
| DOI | 10.1016/j.icarus.2019.06.024 |
| Volume Number | 333 |
| Alternate Webpage(s) | http://www.planetary.brown.edu/pdfs/5232.pdf |
| Language | English |
| Access Restriction | Open |
| Content Type | Text |
| Resource Type | Article |
