NASA has published 600 high resolution photos of the surface of Mars. The images are so detailed that items as small as a writing desks are easily distinguishable.
© NASA . /JPL-Caltech/University of ArizonaNASA has published 600 high resolution photos of the surface of Mars. The images are so detailed that items as small as a writing desks are easily distinguishable.
Photo: The Cerberus Fossae, a series of fissures on Mars.
Photo: The Cerberus Fossae, a series of fissures on Mars.
NASA has published 600 high resolution photos of the surface of Mars. The images are so detailed that items as small as a writing desks are easily distinguishable.
Photo: The Cerberus Fossae, a series of fissures on Mars.
Photo: The Cerberus Fossae, a series of fissures on Mars.
© NASA . /JPL-Caltech/University of ArizonaThe images were taken by the HiRISE camera on board the Mars Reconnaissance Orbiter (MRO) between April 5 and May 6, 2010. A large number of craters can be seen in one of the pictures, which was taken in the middle latitudes of the planet.
The images were taken by the HiRISE camera on board the Mars Reconnaissance Orbiter (MRO) between April 5 and May 6, 2010. A large number of craters can be seen in one of the pictures, which was taken in the middle latitudes of the planet.
© NASA . /JPL-Caltech/University of ArizonaThe Ius Chasma in Valles Marineris is a giant system of canyons. Many scientists believe that Valles Marineris was formed by global cooling.
The Ius Chasma in Valles Marineris is a giant system of canyons. Many scientists believe that Valles Marineris was formed by global cooling.
© NASA . /JPL-Caltech/University of ArizonaGullies on the side of an unnamed crater in the Noachis Terra region can be seen in this image. Scientist believe the gullies were formed from the freezing of drained water.
Gullies on the side of an unnamed crater in the Noachis Terra region can be seen in this image. Scientist believe the gullies were formed from the freezing of drained water.
© NASA . /JPL-Caltech/University of ArizonaA crater on the plain of Meridiani Planum, which is located in the northern upland region of Mars, halfway between the Tharis volcanic region in the west and the Hellas Impact Basin in the south-east.
A crater on the plain of Meridiani Planum, which is located in the northern upland region of Mars, halfway between the Tharis volcanic region in the west and the Hellas Impact Basin in the south-east.
© NASA . /JPL-Caltech/University of ArizonaThe Proctor Crater, located in the southern hemisphere of Mars.
The Proctor Crater, located in the southern hemisphere of Mars.
© NASA . /JPL-Caltech/University of ArizonaThe dunes of Samara Valles, stretching for more than 1,000 kilometers, can be distinguished in this image.
The dunes of Samara Valles, stretching for more than 1,000 kilometers, can be distinguished in this image.
© NASA . /JPL-Caltech/University of ArizonaThis region may become a future landing zone for rocket launches to Mars.
This region may become a future landing zone for rocket launches to Mars.
© NASA . /JPL-Caltech/University of ArizonaLines on the walls of craters, hills and other slopes on Mars
Lines on the walls of craters, hills and other slopes on Mars