Google+ Mars Travel: Aram Chaos
Showing posts with label Aram Chaos. Show all posts
Showing posts with label Aram Chaos. Show all posts

Mars Photo of the Day - May 8 2012

Today's Image of Mars shows a potential landing site for future missions to Mars in Trouvelot Crater. Trouvelot Crater is 154.7km in diameter and located in Oxia Palus Quadrangle, which is known for an abundance of chaos terrain, like Aram Chaos, and numerous outflow channels, most prominently Ares Valles.

Trouvelot Crater is being considered as a possible landing site for the the 2018 joint ESA-Roscosmos ExoMars Rover. One of the features that intrigues scientists are the sedimentary deposits on the crater floor, that many believe could only have been deposited by an abundance of water. On the ground study of these sediments would be able to determine when and how long there was water on the surface and could even provide insight as to where the water went.

Click on this image to see all the other potential landing sites for the ExoMars Rover showcased by Mars Travel.

Credit: HiRISE

Mars Photo of the Day - Jan 17 2012

Today's Image of Mars shows Aram Chaos in false color, as taken by Mars Odyssey Orbiter's THEMIS camera. Aram Chaos is a 280km wide basin in Western Arabia Terra formed over four billion years ago when a huge asteroid hit the surface.

Over millions of years material filled the crater. Because the Martian environment was much wetter the material became saturated with water. As the climate changed the water froze, but then something strange happened. The ice melted. Scientists aren't sure what caused the ice to melt, but they believe that molten rock moved into the ground below the basin.

When the water-ice melted all the sediments that were frozen with it collapsed and formed the chaotic network of valleys, mesas, and hills you see below. The melted water-ice began pooling in the basin and eventually overflowed the eastern basin rim. When the water rose above the eastern rim it created a channel measuring 15km wide, 80km long, and 2500m deep, flowing into Ares Valles.

After the formation of all this chaotic terrain, Aram refilled with water. The water deposited sediments over the chaos terrain. These sediments varied in composition, leading scientists to believe the environment was in a state of transition.

Hematite is abundant in Aram Chaos; in fact, it contains the second largest known deposit on Mars, after Meridiani Planum. Hematite usually forms in association with water, so it's no surprise that scientists were interested in investigating the area in hopes of finding evidence of water on Mars. In fact, scientists were so interested in examining hematite that they sent Mars Exploration Rover Opportunity to Meridiani Planum, where it found the now infamous blueberries, which are hematite-rich nuggets that formed within water-saturated sediments. It's safe to assume that similar features would exist in Aram.

The OMEGA instrument on board Mars Express has more recently detected large deposits of sulfates in Aram. Like Hematite, sulfates are usually formed in the presence of water, which lends credence to the previous conclusions that water was once abundant in Aram Chaos.

Aram Chaos has a long fascinating history and it promises to continue producing surprises as scientists begin to learn more about the conditions under which it was formed.

This image comes from THEMIS aboard the Mars Odyssey Orbiter. Clicking on the image will take you to the original high resolution image from THEMIS. To see their article on Aram Chaos click here.



Mars Photo of the Day - Nov 3 2011

Today's Image of Mars shows a mesa on the eastern floor of Aram Chaos, a 1300km (~800mi) diameter depression. (A mesa is a hill/mountain with a flat top) It is thought that a cataclysmic amount of water was released from this depression, which led to the creation of the 2000km long outflow channel, Ares Vallis.

Surrounding the center mesa you can see many isolated hills and eroding mesas. A variety of dune fields are visible in this image. The interplay between the dunes, eroded land forms, and light and dark-toned materials enables scientists to determine the relative age of each feature, as well as the composition of the interacting materials.

Clicking on this image will take you to a related, captioned image by HiRISE. This image is a subimage of that captioned image.