Knobs near Reull Vallis
NASA/JPL/UArizona
Knobs near Reull Vallis
ESP_017286_1430  Science Theme: Geologic Contacts/Stratigraphy
This observation shows a knob and large crater near Reull Vallis, east of the Hellas Basin. The crater's ejecta blanket abuts the base of the knob. The crater floor and ejecta are blanketed with an ice-rich mantle that is common throughout the Martian mid-latitudes.

The mantle deposits are pitted and grooved perhaps due to the sublimation of ice. This mantle is thought to have been deposited as snow around 10 million years ago during a period of high obliquity, when the planet's axis was more tilted and environmental conditions could have been more conducive to snowfall in these regions.

Several small impact craters are visible on the ejecta blanket that appear to have been filled with mantling deposits that have since been partially removed. These craters give us clues to the erosional history of the deposit. Note the fresh looking impact crater at the top of the knob. This crater does not appear to contain mantling deposits and may be much younger.

This region contains many mesas surrounded by lobate debris aprons that are thought to be ice-rich. These aprons have been interpreted as a variety of possible features including rock glaciers, ice-rich mass movements, or debris-covered glacial flows. Reull Vallis itself is filled with what is referred to as "fretted terrain," which is also thought to be ice-rich material.



Written by: Dan Berman  (5 May 2010)
 
Acquisition date
04 April 2010

Local Mars time
15:19

Latitude (centered)
-36.446°

Longitude (East)
111.212°

Spacecraft altitude
251.3 km (156.2 miles)

Original image scale range
50.3 cm/pixel (with 2 x 2 binning) so objects ~151 cm across are resolved

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50 cm/pixel and North is up

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Equirectangular

Emission angle
0.0°

Phase angle
76.8°

Solar incidence angle
77°, with the Sun about 13° above the horizon

Solar longitude
73.0°, Northern Spring

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Sub-solar azimuth:  50.5°
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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.