On the Floor of the Labyrinth of the Night
On the Floor of the Labyrinth of the Night
PSP_006969_1725  Science Theme: Composition and Photometry
This image shows part of Noctis Labyrinthus, the “Labyrinth of the Night.” This is a system of connecting troughs which form a maze-like network at the western end of Valles Marineris, the giant canyon system of Mars.

The individual troughs are usually kilometers across; this image shows part of the floor of one of the troughs, with some intriguing fine-scale features.

Near the center of the image, the floor is broken up into many small knobs and hills, probably eroded remnants of a larger geologic unit. The most striking feature of many of these knobs is a thin, bright band which often wraps around the edges near the bottom. This image was acquired in order to investigate whether this is an exposed layer of rock or the shoreline of a former body of water.

HiRISE resolves details of the bright band that indicate that this is an unusual layer of rock, rather than an old shoreline. In several places, the band is broken up along cracks, sometimes forming boulders. This indicates that the band is solid rock, while material left on a shoreline should be loose sediments. It is now exposed as rings and arcs where erosion has cut deeply enough to expose the layer.

This band must indicate some unusual event in the geologic history of the region when a different type of rock was deposited; it is strikingly different in color from the other rocks. Although it is not a shoreline, it could be material that was deposited on the floor of a much older lake or sea and then buried by other rock; it could also have been laid down by other sedimentary processes or as volcanic ash.

Written by: Colin Dundas  (27 February 2008)

This is a stereo pair with ESP_028093_1725.
Acquisition date
21 January 2008

Local Mars time

Latitude (centered)

Longitude (East)

Spacecraft altitude
258.7 km (160.8 miles)

Original image scale range
26.3 cm/pixel (with 1 x 1 binning) so objects ~79 cm across are resolved

Map projected scale
25 cm/pixel and North is up

Map projection

Emission angle

Phase angle

Solar incidence angle
42°, with the Sun about 48° above the horizon

Solar longitude
20.7°, Northern Spring

For non-map projected images
North azimuth:  97°
Sub-solar azimuth:  27.2°
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Black & white is 5 km across; enhanced color about 1 km
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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.