The Dark Spot on Mars
NASA/JPL-Caltech/UArizona
The Dark Spot on Mars
ESP_013951_1955  Science Theme: Geologic Contacts/Stratigraphy
On 13 October 1659, Dutch astronomer Christiaan Huygens turned one of his telescopes towards a bright orange spot in the sky and produced what Percival Lowell would later call “the first drawing of Mars worthy of the name ever made by man.” Huygens included a dark spot in his drawing that is thought to represent Syrtis Major, a small sliver of which is visible in this HiRISE image.

Syrtis Major is a shield volcano. Its dark color comes from the dark basaltic rock in the area, visible because it lacks the dust that paints the rest of the planet its distinct, rusty red color. Tracking this dark spot in repeated observations, Huygens concluded that Mars rotated every twenty-four hours: a time not too far off from its true rotation period of approximately 24 hours and 39.58 minutes.

In this image of Syrtis Major, ancient Noachian bedrock is exposed. This is rock made in the early days of Martian history. An impact crater (about 50 kilometers in diameter, or 30 miles) into this rock exposes layers along its wall. These layers may be made from several different geologic materials, such as lava flows, debris from nearby impact craters, or deposits of dust or sand. They may represent different periods of deposition and erosion. The layers are of varying thickness: some of the lighter, resistant units are less than 10 meters thick, while some of the darker layers are over 100 meters thick.

Written by: Andrea Philippoff Jones  (23 December 2009)

This is a stereo pair with ESP_020254_1955.
 
Acquisition date
18 July 2009

Local Mars time
14:22

Latitude (centered)
15.512°

Longitude (East)
72.814°

Spacecraft altitude
275.4 km (171.1 miles)

Original image scale range
55.6 cm/pixel (with 2 x 2 binning) so objects ~167 cm across are resolved

Map projected scale
50 cm/pixel and North is up

Map projection
Equirectangular

Emission angle
8.5°

Phase angle
43.7°

Solar incidence angle
50°, with the Sun about 40° above the horizon

Solar longitude
305.6°, Northern Winter

For non-map projected images
North azimuth:  97°
Sub-solar azimuth:  321.3°
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   (498MB)

IRB color
map-projected   (247MB)

JP2 EXTRAS
Black and white
map-projected  (271MB)
non-map           (249MB)

IRB color
map projected  (106MB)
non-map           (250MB)

Merged IRB
map projected  (505MB)

Merged RGB
map-projected  (469MB)

RGB color
non map           (232MB)
ANAGLYPHS
Map-projected, reduced-resolution
Full resolution JP2 download
Anaglyph details page

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.