On Bond Crater’s Northern Slope
NASA/JPL-Caltech/UArizona
On Bond Crater’s Northern Slope
ESP_074246_1475  Science Theme: Fluvial Processes
This image shows (part of ) a 6-kilometer crater located on the northern slope of Bond Crater. Pole-facing gullies have eroded the northern slope of this small crater, located just west of where Uzboi Valles emanates from Bond and continues in a northerly direction.

However, Hale Crater to the south has numerous gullies on its slopes and even on its central peak region. Researchers have analyzed both Bond and Hale Craters to try to determine why Bond has no gullies on its slopes, except for a small 7-km crater on the floor in its central area. (Reiss et al., 2009, PSS).

The gullies in this observation have eroded into bedrock layers forming tributaries in the upper slope region and distributary channels further downslope on the debris fans. Research attributes these features to fluvial processes. (Gulick et al., 2018, Geol. Soc. London.)

Written by: Ginny Gulick  (24 August 2022)

This is a stereo pair with ESP_074391_1475.
 
Acquisition date
29 May 2022

Local Mars time
15:34

Latitude (centered)
-32.132°

Longitude (East)
323.744°

Spacecraft altitude
257.4 km (160.0 miles)

Original image scale range
26.2 cm/pixel (with 1 x 1 binning) so objects ~78 cm across are resolved

Map projected scale
25 cm/pixel and North is up

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Equirectangular

Emission angle
9.2°

Phase angle
58.0°

Solar incidence angle
49°, with the Sun about 41° above the horizon

Solar longitude
236.6°, Northern Autumn

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North azimuth:  96°
Sub-solar azimuth:  5.1°
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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.