Spider Webs
NASA/JPL/University of Arizona
Spider Webs
ESP_046359_1250  Science Theme: Volcanic Processes
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This image shows a lava channel north of Kuiper Crater in the high southern latitudes just before spring equinox. It was a target suggested by members of the public, using our suggestion tool called HiWish.

The channel confluence at the top of the image illustrates interesting volcanic processes that took place long ago. However, it was the mounds on the rim of the channel to the south of the confluence that we initially found alarming. These mounds, up to 400 meters in diameter, are decorated by radial and concentric patterns that resemble spider webs.

Radial and concentric fractures are familiar from forces penetrating a brittle layer, such as a rock thrown through a glass window. These particular fractures were evidently produced by something emerging from below the brittle surface of Mars. It seems likely that ice lenses, resulting from the accumulation of ice beneath the surface, created these peculiar mounds. Ice is less dense than rock, so the buried ice rose and pushed upwards on the surface and generated these spider web-like patterns. An analogous process creates similar sized mounds in arctic tundra on Earth that are known as “pingos,”, an Inuit word. The Martian fractures in this location are nowadays filled with dust instead of ice, so it is unclear how long ago this activity took place. It seems likely that these pingo-forming periglacial processes took place much more recently than the volcanic activity also evident in this region of Mars.

Written by: Paul Geissler (audio: Tre Gibbs)  (19 October 2016)
 
Acquisition date
16 June 2016

Local Mars time:
15:38

Latitude (centered)
-54.737°

Longitude (East)
202.716°

Spacecraft altitude
249.1 km (155.7 miles)

Original image scale range
49.8 cm/pixel (with 2 x 2 binning) so objects ~150 cm across are resolved

Map projected scale
50 cm/pixel and North is up

Map projection
Equirectangular

Emission angle:
0.3°

Phase angle:
74.3°

Solar incidence angle
74°, with the Sun about 16° above the horizon

Solar longitude
170.1°, Northern Summer

For non-map projected images
North azimuth:  97°
Sub-solar azimuth:  38.8°
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JP2 EXTRAS
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map-projected  (156MB)
non-map           (226MB)

IRB color
map projected  (77MB)
non-map           (246MB)

Merged IRB
map projected  (434MB)

Merged RGB
map-projected  (391MB)

RGB color
non map           (218MB)
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/University of Arizona

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.