Google+ Mars Travel: Weekend Feature
Showing posts with label Weekend Feature. Show all posts
Showing posts with label Weekend Feature. Show all posts

Weekend Feature: Gale Crater

Looking down on Mars we see Gale Crater as a crater among many craters, but even from this distant perspective Gale Crater is unique, special, and above all, intriguing. In the image below we can spot the 150km in diameter Gale Crater because of its massive central uplift, Mount Sharp, which rises 5.5 km above the northern crater floor and 4.5 km above the southern crater floor. It is Mount Sharp that makes Gale Crater so intriguing and worthy of future study.


Mount Sharp's base is thought to be at least 2 billion years old. It is comprised of clays and sulfates, two materials that are only known to form in the presence of water. The layers directly on top of those are comprised primarily of sulfates, with very few clays, which implies that they were formed in an environment where Mars was becoming drier and water was evaporating. See the next image for an idea of what these intriguing layers look like.

Weekend Feature: Arsia Mons

Arsia Mons measures nearly 16km (12mi) high and over 435km (270mi) wide, with a caldera (opening) measuring 110km (72mi) in diameter It is the southernmost of the Tharsis Trio, which also consists of Pavonis Mons to the north and Ascraeus Mons to the north of that.

While Arsia Mons may be larger than any volcano on Earth, it pales in comparison to the largest volcano yet discovered in the solar system, Olympus Mons, which measures 22km (16mi) high. Coincidentally Olympus Mons is relatively close to the Tharsis Trio (right).

These volcanoes lie in the Tharsis Quadrangle on Mars, which contains an abundance of volcanoes. The region is thought to have been volcanically active as recently as 100-250 million years ago, which is relatively recent in geological terms.Scientists believe that the abundance of volcanoes in this region had an astronomical impact on the climate of Mars because the carbon dioxide and water vapor emitted from them would have been enough to create an atmosphere thicker than that on Earth!

This means that the environment we currently see on Mars may be drastically different than what it used to be! The Tharsis volcanoes would have had a direct impact on that, so determining how long ago they were active will help scientists to determine at which point the Martian climate changed!