Edge of the Olympus Mons
NASA/JPL-Caltech/UArizona
Edge of the Olympus Mons
PSP_002184_2005  Science Theme: Mass Wasting Processes
Olympus Mons, the largest volcano in the Solar System, has a mysterious halo (aureole) of material on its western and northern sides. There have been many ideas about how this feature may have formed over the years, but the hypothesis that this is a giant landslide deposit has gained favor.

Many large volcanoes on the Earth collapse under their own weight, so it seems reasonable that Olympus Mons would do the same. The edge of the aureole is seen at the top (northern) part of the image.

It is interesting that the main part of the aureole seems sunk down compared to the edge. It is possible that the ridge along the outer margin of the aureole formed as the flow turned around after pushing uphill for a ways. Imagine a giant wave of rock pushing up onto the "beach" and then receding. It might leave a deposit like this.

Alternatively, glaciers push up a ramp of rock at their fronts. After they retreat, the ridge of rock is left at the furthest extent of the glacier. These are called "terminal moraines" by geologists.



Written by: Laszlo Kestay  (30 May 2007)

 
Acquisition date
13 January 2007

Local Mars time
15:36

Latitude (centered)
20.088°

Longitude (East)
219.712°

Spacecraft altitude
281.9 km (175.2 miles)

Original image scale range
56.5 cm/pixel (with 2 x 2 binning) so objects ~169 cm across are resolved

Map projected scale
50 cm/pixel and North is up

Map projection
Equirectangular

Emission angle
2.7°

Phase angle
51.7°

Solar incidence angle
54°, with the Sun about 36° above the horizon

Solar longitude
166.1°, Northern Summer

For non-map projected images
North azimuth:  97°
Sub-solar azimuth:  359.2°
JPEG
Black and white
map projected  non-map

IRB color
map projected  non-map

Merged IRB
map projected

Merged RGB
map projected

RGB color
non-map projected

JP2
Black and white
map-projected   (133MB)

IRB color
map-projected   (69MB)

JP2 EXTRAS
Black and white
map-projected  (55MB)
non-map           (73MB)

IRB color
map projected  (18MB)
non-map           (60MB)

Merged IRB
map projected  (120MB)

Merged RGB
map-projected  (123MB)

RGB color
non map           (57MB)
ADDITIONAL INFORMATION
B&W label
Color label
Merged IRB label
Merged RGB label
EDR products
HiView

NB
IRB: infrared-red-blue
RGB: red-green-blue
About color products (PDF)

Black & white is 5 km across; enhanced color about 1 km
For scale, use JPEG/JP2 black & white map-projected images

USAGE POLICY
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:
NASA/JPL-Caltech/UArizona

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.