Gale Crater’s small mesas were formed by wind, not liquid water
The Murray Buttes. Click to see August 11, 2016 post.
The uncertainty of science: Though Curiosity has found apparent evidence of past liquid water during its early travels on the floor of Gale Crater, scientists have now concluded that the first small mesas and buttes it traveled past back in 2016, dubbed the Murray Buttes, were not formed by the flow of liquid water but by wind reshaping ancient sand dunes. From the press release:
The lower part of Mount Sharp is composed of ancient lakebed sediments. These sediments accumulated on the lakebed when the crater flooded, shortly after its formation 3.8 billion years ago. Curiosity has spent much of the last nine years investigating these rocks for signs of habitability.
Dr Banham added: “More than 3.5 billion years ago this lake dried out, and the lake bottom sediments were exhumed and eroded to form the mountain at the centre of the crater – the present-day Mount Sharp. The flanks of the mountain are where we have found evidence that an ancient dune field formed after the lake, indicating an extremely arid climate.”
This conclusion comes from a paper released March 30th in the Journal of Geophysical Research: Planets, and uses data obtained by Curiosity from August to September, 2016 (see rover updates from August 11, 2016, from August 28, 2016, and from September 13, 2016).
At that time Curiosity was still on the floor of Gale Crater, where that lake is thought to have once existed, but had reached the first tiny foothills and dune fields that sit at the base of Mt. Sharp.
The scientists also note that this data means that the floor of Gale Crater has not been amicable to life for at least 3 billion years. Dune fields are not places where life prospers, and the Murray Buttes required a lot of time for the original dunes to solidify into the multiple thin layers that exist today.
Click to see August 28, 2016 post.
The photo above illustrates the many thin layers in these buttes. Each layer, only inches thick at most, represents the past existence of a dune anywhere from 13 to 130 feet high that was slowly swept through by Mars’ very thin atmosphere, depositing a new layer behind it. To get that many layers, all squeezed to become soft rock, required a lot of time and many many millions of seasons, during which the environment would have been very hostile to life.
These conclusions also suggest that we really do not yet know what the environment was like in Gale Crater when this theorized past lake existed. This data even suggests that this past liquid water could have been underground, not on the surface, a water table that was liquid because it was not exposed to Mars’ cold and very thin atmosphere.
We do not know, however, since the data available remains very preliminary.
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The Murray Buttes. Click to see August 11, 2016 post.
The uncertainty of science: Though Curiosity has found apparent evidence of past liquid water during its early travels on the floor of Gale Crater, scientists have now concluded that the first small mesas and buttes it traveled past back in 2016, dubbed the Murray Buttes, were not formed by the flow of liquid water but by wind reshaping ancient sand dunes. From the press release:
The lower part of Mount Sharp is composed of ancient lakebed sediments. These sediments accumulated on the lakebed when the crater flooded, shortly after its formation 3.8 billion years ago. Curiosity has spent much of the last nine years investigating these rocks for signs of habitability.
Dr Banham added: “More than 3.5 billion years ago this lake dried out, and the lake bottom sediments were exhumed and eroded to form the mountain at the centre of the crater – the present-day Mount Sharp. The flanks of the mountain are where we have found evidence that an ancient dune field formed after the lake, indicating an extremely arid climate.”
This conclusion comes from a paper released March 30th in the Journal of Geophysical Research: Planets, and uses data obtained by Curiosity from August to September, 2016 (see rover updates from August 11, 2016, from August 28, 2016, and from September 13, 2016).
At that time Curiosity was still on the floor of Gale Crater, where that lake is thought to have once existed, but had reached the first tiny foothills and dune fields that sit at the base of Mt. Sharp.
The scientists also note that this data means that the floor of Gale Crater has not been amicable to life for at least 3 billion years. Dune fields are not places where life prospers, and the Murray Buttes required a lot of time for the original dunes to solidify into the multiple thin layers that exist today.
Click to see August 28, 2016 post.
The photo above illustrates the many thin layers in these buttes. Each layer, only inches thick at most, represents the past existence of a dune anywhere from 13 to 130 feet high that was slowly swept through by Mars’ very thin atmosphere, depositing a new layer behind it. To get that many layers, all squeezed to become soft rock, required a lot of time and many many millions of seasons, during which the environment would have been very hostile to life.
These conclusions also suggest that we really do not yet know what the environment was like in Gale Crater when this theorized past lake existed. This data even suggests that this past liquid water could have been underground, not on the surface, a water table that was liquid because it was not exposed to Mars’ cold and very thin atmosphere.
We do not know, however, since the data available remains very preliminary.
In order to remain completely independent and honest in my writing, I accept no sponsorships from big space companies or any political organizations. Nor do I depend on ads.
Instead, I rely entirely on the generosity of readers to keep Behind the Black running. You can either make a one time donation for whatever amount you wish, or you sign up for a monthly subscription ranging from $2 to $15 through Paypal, or $3 to $50 through Patreon, or any amount through Zelle.
The best method to donate or subscribe is by using Zelle through your internet bank account, since it charges no fees to you or I. You will need to give my name and email address (found at the bottom of the "About" page). What you donate is what I get.
To use Patreon, go to my website there and pick one of five monthly subscription amounts, or by making a one-time donation.
For PayPal click one of the following buttons:
If these electronic payment methods don't work for you, you can support Behind The Black directly by sending your donation by check, payable to Robert Zimmerman, to
Behind The Black
c/o Robert Zimmerman
P.O.Box 1262
Cortaro, AZ 85652
Makes sense to me. With billions of years even a VERY slow process can effect significant change. For instance, consider that a modern semiconductor is manufactured of near invisible circuit elements that measure just 5 nanometers across. So if you assume that wind induced erosion proceeded at something like this scale per year, then given 3 BILLION years you’re looking at 15 meters (~50 feet) of erosion.
Humans simply have a hard time adjusting our perspective to comprehend such a vast expanse of time.
Nice example! And I agree: Humans are not good with very small, very large, very fast, or very slow scales. I roll my eyes when I need to deal with microseconds – I guess I got used to milliseconds during the previous century.