List of evidence for water on Mars |
List of evidence for water on Mars |
Aug 27 2016, 03:14 AM
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#61
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Senior Member Group: Members Posts: 1057 Joined: 17-February 09 Member No.: 4605 |
Well Spirit at Tyrone demonstrated that a thin layer of regolith can provide for a relative humidity gradient protecting hydrated salts. If the regolith is breached then the atmosphere acts as a desiccant. This could explain the appearance and then disappearance of limited amounts of hydrated salts in RSL and would not contradict this latest measurement. Or is could be something else. I suspect it will be a long time before there is consensus on RSL.
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Aug 29 2016, 08:12 PM
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#62
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Member Group: Members Posts: 363 Joined: 13-April 06 From: Malta Member No.: 741 |
A study published discussing inverted river channels in Arabia terra as a sign of a warm and wet climate on early Mars talks about ancient river channels flowing from topographic highs to lower regions from south to the lower northern regions. My question is where would meridiani planum fit along this topographic gradient? The rocks stu died by opportunity rover were mainly sulphate rocks suggestive of acidic water alteration . The inverted channels discussed seem to originate on early mars where water would be expected to form different rock types from those observed by opportunity! Maybe I am getting the ages wrong. Correct me if I am wrong.
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May 9 2019, 12:48 AM
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#63
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Senior Member Group: Members Posts: 1057 Joined: 17-February 09 Member No.: 4605 |
The linked Planetary Society blog article provides an interesting read on the faint young sun paradox with respect to long lived surface water on early Mars and puts to bed some of the hypothetical explanations. However the article did miss the hypothesis that the solar system transiting through interstellar dust clouds could have the effect of significantly increasing the sun's output through the capture of molecular hydrogen. That hypothesis has always made a lot of sense to me.
http://www.planetary.org/blogs/guest-blogs...le-paradox.html |
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Jun 19 2019, 05:05 PM
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#64
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Member Group: Members Posts: 684 Joined: 24-July 15 Member No.: 7619 |
The linked Planetary Society blog article provides an interesting read on the faint young sun paradox with respect to long lived surface water on early Mars and puts to bed some of the hypothetical explanations. However the article did miss the hypothesis that the solar system transiting through interstellar dust clouds could have the effect of significantly increasing the sun's output through the capture of molecular hydrogen. That hypothesis has always made a lot of sense to me. http://www.planetary.org/blogs/guest-blogs...le-paradox.html I saw two recent papers/references that seem relevant, or at least interesting. FIRST, was a paper on the 11/22 year solar cycle and Jupiter (yes, related to the barycenter theory) which looked at the 11.07 year cycle of solar atmospheric tides that results from Venus-Earth-Jupiter orbital resonances.
https://link.springer.com/article/10.1007/s11207-019-1447-1 So, let's consider that Theory #1 the "solar cycle / planetary barycenter theory" might be correct well, let's consider that Theory #2 "Nice-Model" might be correct as well. In that case, the early Sun had 4 gas giants between ~5 AU and ~17 AU. Resonances would have driven massive solar dynamo effects. Basically, if you have 4 gas giants on circular orbits within ~17 AU, you have tides stirring the Sun and stoking the fire. SECOND is a combination of idea, the mention of lunar GRAIL data that the lunar surface is roughly 15% void space for the first few kilometers, and a review that the breccia and impact melt under Gale crater could be 17 km deep (for comparision, the Marianas Trench on earth is ~11 km deep) with an initial void space of 3,600 cubic kilometers. This suggests that there is plenty of "space" for liquid water to exist in the Martian subsurface. That implies that the real trick about water on the surface of Mars is keeping it from draining back down into the regolith. Perhaps we only see Martian rivers when they run across compacted sediments or permafrost, otherwise, the water quickly soaks into the sand and gravel. Flip the thinking to view rivers on the surface of Mars more like the meltwater channels on the top of a glacier, as soon as they encounter a lens of clean sand or a crack, they are gone. https://phys.org/news/2018-01-glacial-mouli...ered-rapid.html |
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Feb 21 2020, 05:56 PM
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#65
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Member Group: Members Posts: 401 Joined: 5-January 07 From: Manchester England Member No.: 1563 |
I don't know if this has been mentioned before, but the story is on several news outlets, so it seems appropriate to post the original paper here: Crocus melting on Mars:
https://iopscience.iop.org/article/10.3847/1538-4357/ab612f -------------------- |
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Feb 24 2020, 06:35 AM
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#66
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Senior Member Group: Members Posts: 1057 Joined: 17-February 09 Member No.: 4605 |
Here is the complete abstract from the LPSC 2020 Marsbug.
https://www.hou.usra.edu/meetings/lpsc2020/pdf/1792.pdf I believe the last sentence in the abstract is germane. There simply isn't sufficient precipitable water vapor in the atmospheric column to create meaningful brine. |
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Feb 24 2020, 02:17 PM
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#67
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Member Group: Members Posts: 684 Joined: 24-July 15 Member No.: 7619 |
I don't know if this has been mentioned before, but the story is on several news outlets, so it seems appropriate to post the original paper here: Crocus melting on Mars: https://iopscience.iop.org/article/10.3847/1538-4357/ab612f I also thought this was quite interesting- but for a slightly different reason- If a boulder can generate the necessary shadows from positive curved geometry, wouldn't the negative geometry of a crater have a similar effect? Also, a crater would seem to have an advantage of access to absorbed/adsorbed subsurface moisture. |
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Feb 25 2020, 09:49 PM
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#68
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Member Group: Members Posts: 866 Joined: 15-March 05 From: Santa Cruz, CA Member No.: 196 |
You're right we don't hear much on this anymore. I recall that being part of initial speculation when the first gullies were discovered by MGS some 20 years ago. i got a sense that the cold-trap model didnt hold up but nevertheless i still like to armchair-speculate such processes may remain relevant at certain points in Mars' climate intervals to accelerate erosion in applicable places and contribute to such formations.
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Feb 27 2020, 02:11 PM
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#69
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Member Group: Members Posts: 401 Joined: 5-January 07 From: Manchester England Member No.: 1563 |
Just generally, from my physics background, layman's understanding of Martian weather and geology, and following forums and threads like this one, it has always seemed like there's no insurmountable barrier to small amount of transient liquid water forming on present day Mars, when the right conditions come together. But really solid evidence of it seems to be elusive, so perhaps, like me, people are waiting for something really direct and unarguable.
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Mar 16 2021, 11:26 PM
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#70
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Member Group: Members Posts: 311 Joined: 31-August 05 From: Florida & Texas, USA Member No.: 482 |
I'm sharing this LPSC abstract because it is quite interesting: a site that contains deltas, lake sediments, and a possible extinct underwater geyser basin
"A POSSIBLE SUBAQUEOUS HYDROTHERMAL SYSTEM IN MELAS CHASMA, MARS" https://www.hou.usra.edu/meetings/lpsc2021/pdf/2432.pdf |
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Apr 29 2023, 01:13 AM
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#71
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Member Group: Members Posts: 401 Joined: 5-January 07 From: Manchester England Member No.: 1563 |
My apologies for the thread necromancy, but it seems that this paper and any debate on it fits exactly:
Modern water at low latitudes on Mars: Potential evidence from dune surfaces https://www.science.org/doi/10.1126/sciadv.add8868 -------------------- |
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Apr 30 2023, 04:21 PM
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#72
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Member Group: Members Posts: 684 Joined: 24-July 15 Member No.: 7619 |
My apologies for the thread necromancy, but it seems that this paper and any debate on it fits exactly: Modern water at low latitudes on Mars: Potential evidence from dune surfaces https://www.science.org/doi/10.1126/sciadv.add8868 Interesting summary Snows or frosts possible as recently as 1.4 million years ago to 440,000 years ago. QUOTE (Modern water at low latitudes on Mars) Abstract
Landforms on the Martian surface are critical to understanding the nature of surface processes in the recent past. However, modern hydroclimatic conditions on Mars remain enigmatic, as explanations for the formation of observed landforms are ambiguous. We report crusts, cracks, aggregates, and bright polygonal ridges on the surfaces of hydrated salt-rich dunes of southern Utopia Planitia (~25°N) from in situ exploration by the Zhurong rover. These surface features were inferred to form after 1.4 to 0.4 million years ago. Wind and CO2 frost processes can be ruled out as potential mechanisms. Instead, involvement of saline water from thawed frost/snow is the most likely cause. This discovery sheds light on more humid conditions of the modern Martian climate and provides critical clues to future exploration missions searching for signs of extant life, particularly at low latitudes with comparatively warmer, more amenable surface temperatures. |
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May 3 2023, 12:39 PM
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#73
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Senior Member Group: Members Posts: 1057 Joined: 17-February 09 Member No.: 4605 |
This is in accord with modeled changes in the obliquity of Mars as below, resulting in cyclical sublimation and deposition of the ice caps. At higher obliquities the poles receive greater insolation and the CO2/water vapor content of the atmosphere increases. The increased greenhouse effect would cause a degree of warming with higher pressure and humidity resulting in deposition of water ice in the cooler, lower latitudes. I assume the 1.4 to 0.4 million year timescale for the features imaged by Zhurong is based on the last modeled obliquity sequence which indicates 7 or 8 cycles.
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Mar 21 2024, 06:14 PM
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#74
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Member Group: Members Posts: 708 Joined: 1-April 08 From: Minnesota ! Member No.: 4081 |
Not sure if this is the best topic for this post or if other members have posted this elsewhere already. Anyway, I noticed a SETI Institute Press Release of a presentation at the 54th LPSC concerning the identification of a newly discovered giant volcano on Mars located just south of the planet’s equator, in Eastern Noctis Labyrinthus and west of Valles Marineris. https://www.seti.org/press-release/giant-vo...discovered-mars. The authors’ abstract is here https://www.hou.usra.edu/meetings/lpsc2024/pdf/2745.pdf. I believe this is the same group that presented an abstract at the 53rd LPSC concerning a ‘relict glacier’ in this region. https://www.seti.org/press-release/remains-...t-low-latitudes
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Jun 13 2024, 01:27 AM
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#75
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Member Group: Members Posts: 316 Joined: 1-October 06 Member No.: 1206 |
Water frost deposition in the Calderas of Martian Tharsis volcanoes esp Olympus Mons.
https://www.nature.com/articles/s41561-024-01457-7 P |
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