Unravelling Part of Olympus Monsí Geologic History
NASA/JPL/University of Arizona
Unravelling Part of Olympus Monsí Geologic History
PSP_006891_1970  Science Theme: Volcanic Processes
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Olympus Mons is the largest volcano in the Solar System. While it is one of the youngest volcanoes on Mars, it has a complicated history. This image reveals new details of the sequence of geologic events around its base.

At the top of the cutout, there is a large hill that is surrounded by lava flows from Olympus Mons. This hill is likely to be a chunk of the older part of the volcano that was moved here by a large land slide. The lava flows along the flank of Olympus Mons had most of the lava transported through channels. These channels are preserved where the lava drained out from between the stationary walls (called "levees," like along the sides of a contained river).

The bottom right part of the cutout has a much flatter and smoother surface. These are younger lava flows that have buried the lower part of the volcano. When lava flows form vast smooth sheets, they are called "flood" lavas.

In the bottom of the cutout, the flood lavas have odd, wiggly looking plateaus. These are parts of the lava crust that were lifted up when more liquid lava was injected into the middle of the slowly solidifying lava flow. This process is called "inflation" and is seen on many lava flows on Earth. These younger lava flows are cut by two different sets of faults. One makes the branching valley in the flood lavas and the other creates the sinuous ridge and valley along the edge of the Olympus Mons lava flows. Lower resolution images that cover a broader area suggest that the sinuous fault is an old buried structure that has been more recently reactivated.

Written by: Laszlo P. Keszthelyi  (20 February 2008)

This is a stereo pair with ESP_011519_1970.
 
Acquisition date
15 January 2008

Local Mars time
14:32

Latitude (centered)
16.887°

Longitude (East)
231.036°

Spacecraft altitude
277.0 km (172.1 miles)

Original image scale range
55.4 cm/pixel (with 2 x 2 binning) so objects ~166 cm across are resolved

Map projected scale
50 cm/pixel and North is up

Map projection
Equirectangular

Emission angle
0.2°

Phase angle
38.3°

Solar incidence angle
38°, with the Sun about 52° above the horizon

Solar longitude
17.8°, Northern Spring

For non-map projected images
North azimuth:  97°
Sub-solar azimuth:  356.6°
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All of the images produced by HiRISE and accessible on this site are within the public domain: there are no restrictions on their usage by anyone in the public, including news or science organizations. We do ask for a credit line where possible:
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POSTSCRIPT
NASA’s Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, Calif., manages the Mars Reconnaissance Orbiter for NASA’s Science Mission Directorate, Washington. The HiRISE camera was built by Ball Aerospace and Technology Corporation and is operated by the University of Arizona.