Elysium Planitia, located in the Elysium and Aeolis quadrangles, is a broad plain that straddles the equator of Mars, centered at 3°00′N154°42′E / 3.0°N 154.7°E / 3.0; 154.7.[1] It lies to the south of the volcanic province of Elysium, the second largest volcanic region on the planet, after Tharsis. Elysium contains the major volcanoes Elysium Mons, Albor Tholus and Hecates Tholus. Another more ancient shield volcano, Apollinaris Mons, is situated just to the south of eastern Elysium Planitia. Within the plains, Cerberus Fossae is the only Mars location with recent volcanic eruptions. Lava flows dated no older than 0.2 million years from the present have been found,[2] and evidence has been found that volcanic activity may have occurred as recently as 53,000 years ago. Such activity could have provided the environment, in terms of energy and chemicals, needed to support life forms.[3][4]
The largest craters in Elysium Planitia are Eddie, Lockyer, and Tombaugh. The planitia also has river valleys—one of which, Athabasca Valles may be one of the youngest on Mars. On the north east side is an elongated depression called Orcus Patera, and this and some of the eastern plains were imaged in the 1965 Mariner 4 flyby.[5]
A 2005 photo of a locale in Elysium Planitia at 5°N, 150°E by the Mars Express spacecraft shows what may be ash-covered water ice. The volume of ice is estimated to be 800 km (500 mi) by 900 km (560 mi) in size and 45 m (148 ft) deep, similar in size and depth to the North Sea.[6] The ice is thought to be the remains of water floods from the Cerberus Fossae fissures about 2 to 10 million years ago. The surface of the area is broken into 'plates' like broken ice floating on a lake (see below). Impact crater counts show that the plates are up to 1 million years older than the gap material, showing that the area solidified much too slowly for the material to be basaltic lava.[7]
NASA'sInSight mission landed in Elysium Planitia on 26 November 2018.[8] It took off from Earth on 5 May 2018. The probe will study the internal structure of Mars and by so doing improve understanding of the planet's evolution. InSight Mars lander was able to take color pictures from the surface Elysium Planitia and sent them by radio signal back to Earth. During the descent sequence two additional items were jettisoned, the backshell with parachute, and heat shield, and they impacted in the vicinity of the lander.
First images of Elysium Planitia from InSight's Instrument Context Camera (ICC, left), without lens cover and stretched (ICC, Middle), and the Instrument Deployment Camera (IDC, right)
All the originally proposed landing sites are in Elysium Planitia; this ellipse, located at 4°30′N136°00′E / 4.5°N 136°E / 4.5; 136, represents the site finally selected.
Image footprints by HiRise on Mars Reconnaissance Orbiter for studying the planned Insight landing ellipse. From east to west the scale is about 160 km (100 mi).
InSight final landing location (red dot) (13 December 2018)
InSight backshell with parachute, lander, heat shield (11 December 2018)
InSight backshell with parachute, lander, heat shield (26 November 2018)
Wide view of layered buttes and small mesas, as seen by HiRISE under HiWish program. Some dark slope streaks are visible.
Layered mesa and mounds with dark slope streaks, as seen by HiRISE under HiWish program
Close view of layered small mesa with dark slope streak, as seen by HiRISE under HiWish program. Box shows the size of a football field.
Very close view of individual blocks breaking off layer in a butte, as seen by HiRISE under HiWish program Blocks have angular shapes. Box shows size of football field.
Layered mesas, as seen by HiRISE under HiWish program
Layered mesas, as seen by HiRISE under HiWish program. Dark slope streaks are also visible.
Mesas, as seen by HiRISE under HiWish program. Top layer; the cap rock is breaking up into boulders.
Close view of cap rock breaking up into boulders, as seen by HiRISE under HiWish program
MOLA map showing boundaries of Elysium Planitia and other nearby regions
Layers around streamlined knob, as seen by HiRISE under HiWish program
Layers in old crater rim, in Marte Vallis as seen by HiRISE under HiWish program
Close view of layers from previous image, as seen by HiRISE under HiWish program. Some dark slope streaks are visible.
Mounds with layers, as seen by HiRISE under HiWish program. Location is east of Gale Crater in the Aeolis quadrangle.
These icy plates moved to the left, and obstacles (crater rims) turned them into piles of pieces.
Mound showing layers at the base, as seen by HiRISE under HiWish program. Location is east of Gale Crater in the Aeolis quadrangle.
Yardangs showing layers, as seen by HiRISE under HiWish program. Location is east of Gale Crater in the Aeolis quadrangle.
Mesas and eroded parts of mesas showing layers and dark slope streaks, as seen by HiRISE under HiWish program. Image is located in eastern Avernus Colles.
Wide view of layered terrain, as seen by HiRISE under HiWish program. Location is northeast of Gale Crater.
Close view of mound with layers, as seen by HiRISE under HiWish program. Note: this is an enlargement from the previous image.
Close view of mound with layers, as seen by HiRISE under HiWish program. Note: this is an enlargement from a previous image.
Wide view of layered terrain, as seen by HiRISE under HiWish program. Note: parts of this image are enlarged in the next three images.
Close view of layers in a mound, from previous image, as seen by HiRISE under HiWish program
Close view of layers in a mound, from a previous image, as seen by HiRISE under HiWish program
Close view of layers in a mound, from a previous image, as seen by HiRISE under HiWish program
Lava field on Elysium Planitia resembling an elephant
Lava flow and dark slope streaks, as seen by HiRISE under HiWish program
^Golombek, M.; et al. (2017). Selection of the 2018 Insight Landing Site. 48th Lunar and Planetary Science Conference. 20–24 March 2017. The Woodlands, Texas. Bibcode:2017LPI....48.1515G. LPI Contribution No. 1964, id.1515.
Interactive image map of the global topography of Mars. Hover your mouse over the image to see the names of over 60 prominent geographic features, and click to link to them. Coloring of the base map indicates relative elevations, based on data from the Mars Orbiter Laser Altimeter on NASA's Mars Global Surveyor. Whites and browns indicate the highest elevations (+12 to +8 km); followed by pinks and reds (+8 to +3 km); yellow is 0 km; greens and blues are lower elevations (down to −8 km). Axes are latitude and longitude; Polar regions are noted. 
