Анаглифы поверхности Марса

[Kaetano]

Берём вот такие очки:

... и наслаждаемся видами Марса.


Долины и кратеры:

Cydonia Labyrinthus is a complex of intersecting valleys that form a polygonal fractured terrain.


This 3D, or stereo anaglyph, view shows the upcoming science destination for NASA's Mars rover Curiosity, a region dubbed "Glenelg," where three different types of material seen from orbit come together (middle of picture).


Lucus Planum is a part of the enigmatic Medusa Fossae Formation, a broad, soft, and easily eroded deposit. Here this deposit is thin and considerably rougher than elsewhere, implying that it is heavily eroded. Here a channel can be seen cutting into this deposit.



Mawrth Vallis is one of the oldest valleys on Mars, formed in and subsequently covered by layered rocks, which are now exposed due to erosion. Mars orbiters have observed clay minerals that form in water in and surrounding this valley, which made Mawrth Vallis one of the locations considered as a landing site for the Curiosity rover. Multiple impact craters within this image have been partially filled in by wind-blown sand


Mawrth Vallis contains clay minerals that formed by chemical alteration of rocks by water. The central part of the image is dominated by light-toned materials with curving fractures of many different sizes. These fractures do not have a preferred orientation, indicating that they probably formed by the drying of a thick mud deposit or the gradual rebound of the area as the overlying material was eroded away. The impact crater on the left side has been partially filled in by wind-blown sand.


This image features an exhumed crater in Meridiani Planum, an equatorial region where the rover Opportunity has been exploring the Martian surface since January 2004. An exhumed crater is one that was buried after formation, and then exposed at the surface once again by subsequent erosion. Remnants of the layered material that filled this crater can still be seen.


This image shows layered sedimentary rocks and ripples that fill and surround an impact crater in Meridiani Planum, an equatorial region where the rover Opportunity has been exploring the Martian surface since January 2004. These layered deposits may have formed through the accumulation of sediment that were transported into this region by blowing wind or flowing water.


Candor Chasma is one of the major canyons within Valles Marineris. The floor of this canyon consist of many layers of light-toned sediments that have been folded and faulted, giving them the wavy appearance seen in this image.


Tantalus Fossae are a set of faults on the eastern flank of Alba Mons, one of the great Tharsis Montes volcanoes. Here a fault cuts into this crater, indicating that the fault formed after the crater. Material has filled in the crater floor and obscured any trace of the faults running across the crater floor, likely after the fault was active.


Shalbatana Vallis is a large channel with steep walls and a flat floor that may have formed by water draining from nearby Ganges Chasma. Here a section of the wall collapsed and produced a landslide into the valley floor.


Вид с орбиты на марсоход:

This 3D, or stereo anaglyph, view shows NASA's Mars rover Curiosity where it landed on Mars within Gale Crater, at a site now called Bradbury Landing.


Парашют:

This 3D, or stereo anaglyph, view shows the parachute and back shell that helped guide NASA's Curiosity to the surface of Mars.


Возможно, здесь была вода:

This stereo image from the Mast Camera (Mastcam) on NASA's Mars rover Curiosity shows a rock outcrop called "Hottah," cited as evidence for vigorous flow of water in a long-ago Martian stream.


Некая деталь марсохода, назначение которой я не поняла (Mars Hand Lens Imager — ???)

This 3-D view of the calibration target for the Mars Hand Lens Imager (MAHLI) aboard NASA's Mars rover Curiosity was assembled from two images taken by that camera during the 34th Martian day, or sol, of Curiosity's work on Mars (Sept. 9, 2012).


Панорамы с марсоходом:

Left and right eyes of the Navigation Camera (Navcam) in NASA's Curiosity Mars rover took the dozens of images combined into this stereo scene of the rover and its surroundings. The component images were taken during the 166th, 168th and 169th Martian days, or sols, of Curiosity's work on Mars (Jan. 23, 25 and 26, 2013). The scene appears three dimensional when viewed through red-blue glasses with the red lens on the left. It spans 360 degrees, with Mount Sharp on the southern horizon.




NASA's Mars rover Curiosity drove 6.2 feet (1.9 meters) during the 100th Martian day, or sol, of the mission (Nov. 16, 2012).


This 3-D image from NASA's Curiosity was taken from the rover's Bradbury Landing site inside Gale Crater, Mars, using the left and right eyes of its Navigation camera. Between the rover on the right, and its shadow on the left, looms the rover's eventual target: Mount Sharp. The mountain's highest peak is not visible to the rover from the landing site.



Всё отсюда: mars.jpl.nasa.gov/mars3d/
(а ещё тут можно посмотреть крупнее)