Nested Channels near Hellas
NASA/JPL-Caltech/UArizona
Nested Channels near Hellas
ESP_042433_1535  Science Theme: Fluvial Processes
We’re not sure if this channel-inside-a-channel was carved by flowing water or lava. Flowing water erodes channels, and flowing lava both erodes and melts surrounding rock to form channels.

It’s not clear whether a huge surge of water or lava first formed the wide channel and then subsided into a trickle to form this narrow, inner channel, or if a trickle formed the inner channel and a subsequent surge formed the wider one. Detailed analysis of the shape could reveal which scenario is most likely, as well as whether water or lava is responsible. Relevant observations for such a determination would include, for example, the facts that the channels lack levees (ridges along the banks) and that the inner channel diverts around a mound, which at one time was an island.

This channel system flowed to the southwest toward the huge Hellas impact basin.

Written by: Kirby Runyon (narration: Tre Gibbs)  (30 September 2015)

This is a stereo pair with ESP_042855_1535.
 
Acquisition date
15 August 2015

Local Mars time
14:47

Latitude (centered)
-26.398°

Longitude (East)
98.505°

Spacecraft altitude
255.6 km (158.9 miles)

Original image scale range
51.1 cm/pixel (with 2 x 2 binning) so objects ~153 cm across are resolved

Map projected scale
50 cm/pixel and North is up

Map projection
Equirectangular

Emission angle
1.6°

Phase angle
54.6°

Solar incidence angle
56°, with the Sun about 34° above the horizon

Solar longitude
27.9°, Northern Spring

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North azimuth:  97°
Sub-solar azimuth:  44.1°
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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.