Google+ Mars Travel: sediments on Mars
Showing posts with label sediments on Mars. Show all posts
Showing posts with label sediments on Mars. Show all posts

Mars Rock vs Earth Rock - Can You Tell the Difference?

The below image shows us just how difficult it can be to differentiate the surface of Mars from Earth's. This image was taken by MSL Curiosity on 2 Sep 2012, it's 27th sol (Martian day) since it's operation in Gale Crater

Which one is which?

Click to see larger, annotated version from NASA.

Mars Photo of the Day - May 30 2012

Today's Image of Mars shows different minerals exposed along a slope in Coprates Chasma, as imaged by HiRISE. The slope is on the left in this image, while the floor of Coprates Chasma is on the right. The brighter material has been exposed over millions of years of erosion and likely represents minerals that are older than the overlying terrain.

It appears that these minerals were deposited at a time when water or ice was abundant. We can tell this by the composition and layering of the material. The material seems to be of a sedimentary nature and it contains layers that are oftentimes seen in materials deposited by water.

Clicking on this image will take you to the original high resolution image from HiRISE. [See the original HiRISE caption]




Mars Photo of the Day - Jan 16 2012

Today's Image of Mars once again shows Iani Chaos, but this time we can see all the intricate features  created by the massive amount of water that once passed through the area. Iani Chaos was the source for the large outflow channel, Ares Valles after geologic faults ruptured an enormous reservoir of ground water, causing it to flood the surface.

Two Mars orbiters (Mars Global Surveyor and Mars Express) have found mineralogical evidence that there was once an abundance of water in Iani Chaos, lending credence to the idea that the features below were formed by water. The two Mars orbiters found hematite and gypsum in the area, two minerals that are only known to be formed in the presence of an abundance of water.

But how did all these features form?

Looking at the image you can see many web-like features created by what look like inverted riverbeds. Once active rivers on Mars deposited sediments, which were more wear-resistant than the surrounding terrain. When Mars dried up these sediments remained. Over billions of years the wind on Mars eroded the landscape, but the hardened sediments were harder than the surrounding terrain so they became less eroded, thus the reason you see this web of features.

But where did these rivers come from?

When geologic faults ruptured an underground reservoir, millions of tons water poured out onto the surface. The water took the easiest way out, following natural features and creating what we see here today. 

You can see in the bottom right of this image that the terrain is about as high as the inverted riverbeds we see elsewhere. I think we can safely assume from this that there was an enormous presence of water at the bottom right of this image, which drained through the interlocking riverbeds we see below. While this is just an educated guess, these same features are common on Earth, where great lakes and seas have channels and rivers feeding into and out of them.

 Clicking on this image will show the larger size. To see the THEMIS article this image came from
Source: THEMIS

Mars Photo of the Day - Jan 7 2012

Today's Image of Mars was taken by HiRISE and shows us some puzzling ridges in Aureum Chaos. Scientists are unsure of what created this unusual ridged feature, but in an attempt to explain what they are seeing, the HiRISE team has come up with a geological history that would explain the below features. That history is detailed below:

  • Sediments were deposited by water or airfall.
  • Stresses in the sediments created a "crudely polygonal patterned" surface.
  • Ground water navigated the fracture patterns and deposited minerals which cemented the sediments. 
  • After billions of years of wind erosion, the cemented, more wear-resistant fractures were left as the high-standing ridges seen below.
The HiRISE team emphasizes that this is just pure speculation on their part and there is no way to be sure exactly how these high-standing ridges came to be. Click on the image below to see the original captioned image from HiRISE that contains their speculation.


Mars Photo of the Day - Dec 9 2012

Today's Image of Mars shows an inverted, winding, riverbed surrounded by features called yardangs

Yardangs are created when the primary form of erosion is wind. They are easy to identify as they have multiple sharp ridges that are oriented in a similar way: a result of wind erosion over millions of years. 

But why is the riverbed raised? Shouldn't it be carved into the surface?

When the river was flowing it deposited layer after layer of sediments, which were harder than the surrounding terrain. Since the river dried up the whole area has spent millions of years being eroded by wind. Because the sediments deposited by the river bed were harder than the surrounding terrain they were eroded much less than the rest of the surface, thus the reason the river bed is inverted.

Today's image was taken by HiRISE. Clicking on the image will take you to the original captioned image from them!