Ancient Streamlined Islands of the Palos Outflow Channel
NASA/JPL-Caltech/UArizona
Ancient Streamlined Islands of the Palos Outflow Channel
ESP_045782_1820  Science Theme: Fluvial Processes
This image shows the northern terminus of an outflow channel located in the volcanic terrains of Amenthes Planum.

The channel sources from the Palos impact crater to the south, where water flowed into the crater from Tinto Vallis and eventually formed a paleo lake. As rising lake levels breached through the crater’s rim and inundated the plains to the north, the resulting high velocity, large discharge floods plucked out and eroded the volcanic plains scouring out the “Palos Outflow Channel” and the streamlined mesa-islands on its floor.

These streamlined forms are the eroded remnants of plains material sculpted by catastrophic floods and are not sediment deposits emplaced by lower magnitude stream flows. Both the fluvial channel floor and the volcanic island surfaces are densely cratered by impacts suggesting that both the surfaces and the flood events are ancient.

The morphology (shape) of the channel system and its islands have been preserved through the eons, but water has long been absent from this drainage system. Since then, winds have transported light-toned sediments across this terrain forming extensive dune fields within the channel system, on the floors of impact craters, and in other protected locations in the Palos Outflow Channel region.

A closer look shows chevron, or fish-bone shaped, light-toned dunes located near the top of the image where numerous smaller channels have cut through the landscape. These dunes likely started out as Transverse Aeolian Ridges (TAR) that form perpendicular to the prevailing wind direction where the wind-blown sediment supply is scarce. This intriguing morphology likely reflects changes in the prevailing wind environment over time.

Written by: Henrik Hargitai and Ginny Gulick (narration: Tre Gibbs)  (24 August 2016)
 
Acquisition date
02 May 2016

Local Mars time
15:13

Latitude (centered)
2.079°

Longitude (East)
107.530°

Spacecraft altitude
269.8 km (167.7 miles)

Original image scale range
54.3 cm/pixel (with 2 x 2 binning) so objects ~163 cm across are resolved

Map projected scale
50 cm/pixel and North is up

Map projection
Equirectangular

Emission angle
6.6°

Phase angle
55.4°

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

Solar longitude
146.4°, Northern Summer

For non-map projected images
North azimuth:  97°
Sub-solar azimuth:  22.7°
JPEG
Black and white
map projected  non-map

IRB color
map projected  non-map

Merged IRB
map projected

Merged RGB
map projected

RGB color
non-map projected

JP2
Black and white
map-projected   (304MB)

IRB color
map-projected   (168MB)

JP2 EXTRAS
Black and white
map-projected  (168MB)
non-map           (166MB)

IRB color
map projected  (82MB)
non-map           (180MB)

Merged IRB
map projected  (347MB)

Merged RGB
map-projected  (319MB)

RGB color
non map           (170MB)
BONUS
4K (TIFF)

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-Caltech/UArizona

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.