NASA - water on Mars, sediment pictures

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Discussion Overview

The discussion centers around the presence of water on Mars and the implications of sedimentary structures observed by NASA's Curiosity rover. Participants explore the processes of erosion, sediment deposition, and the geological history of Mars, considering both theoretical and observational evidence.

Discussion Character

  • Exploratory, Technical explanation, Debate/contested

Main Points Raised

  • Some participants question the fate of eroded material on Mars, suggesting it may have been carried away by wind.
  • There is a proposal that the eroded material could have been deposited in layers, with references to sedimentary signs indicative of a Martian lakebed.
  • One participant discusses the evidence for a primordial ocean on Mars, noting that while there is significant evidence, it remains inconclusive regarding the planet's atmospheric conditions necessary for liquid water.
  • Another participant raises a question about distinguishing aeolian deposits from lacustrine deposits, indicating a need for clarity in sediment classification.

Areas of Agreement / Disagreement

Participants express various viewpoints on the processes involved in sediment deposition and the historical presence of water on Mars. There is no clear consensus, and multiple competing views remain regarding the geological history and sedimentary processes on Mars.

Contextual Notes

Some claims depend on interpretations of geological evidence and may be influenced by ongoing debates in scientific literature. The discussion reflects uncertainty about the atmospheric conditions on Mars and the classification of sediment types.

Who May Find This Useful

This discussion may be of interest to those studying planetary geology, astrobiology, or the history of water on Mars, as well as enthusiasts of NASA's Mars exploration missions.

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So, where'd the eroded material go?
 
And deposited in a homogeneous mass? Or in layers?
 
Likely deposited in layers. Titled OP link: Sedimentary Signs of a Martian Lakebed | NASA
This is an example of a thick-laminated, evenly-stratified rock type that forms stratigraphically beneath cross-bedded sandstones regarded as ancient river deposits. These rocks are interpreted to record sedimentation in a lake, as part of or in front of a delta, where plumes of river sediment settled out of the water column and onto the lake floor.
 
While there is significant evidence suggesting Mars had a primordial ocean, it remains inconclusive. It does not require a particularly vivid imagination to picture the process that supplied primordial water to Earth would have done the same to mars. The bigger question is likely whether Mars ever had sufficient atmosphere to permit liquid water to accumulate on its surface. Certainly vulcanism is a candidate source for atmospheric gasses on mars. It is fairly obvious Mars underwent an early episode of intense volcanic activity not unlike Earth - which is widely regarded as a major contributor to Earth's primordial atmosphere. The topic is frequently debated in scientific literature For one of the more recent papers see; http://arxiv.org/abs/1411.5144, Estimating precipitation on early Mars using a radiative-convective model of the atmosphere and comparison with inferred runoff from geomorphology. Hopefully, Curiosity will yield further insight.
 
Aeolian deposits from 4.5 Ga of dust storms are distinguished from lacustrine deposits how?
 

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