The Dark Spot on Mars
NASA/JPL/University of Arizona
The Dark Spot on Mars
ESP_013951_1955  Science Theme: Geologic Contacts/Stratigraphy
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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.

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Acquisition date
18 July 2009

Local Mars time:

Latitude (centered)

Longitude (East)

Range to target site
277.7 km (173.6 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

Emission angle:

Phase angle:

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

Solar longitude
305.6°, Northern Winter

North azimuth:

Sub-solar azimuth:
Black and white
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IRB color
map projected  non-map

Merged IRB
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Merged RGB
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RGB color
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Black and white
map-projected   (498MB)

IRB color
map-projected   (247MB)

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

IRB color
map projected  (106MB)
non-map           (248MB)

Merged IRB
map projected  (504MB)

Merged RGB
map-projected  (468MB)

RGB color
non map           (231MB)
Map-projected, reduced-resolution
Full resolution JP2 download
Anaglyph details page

B&W label
Color label
Merged IRB label
Merged RGB label
EDR products

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

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/University of Arizona

For information about NASA and agency programs on the Web, visit: 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. Lockheed Martin Space Systems is the prime contractor for the project and built the spacecraft. The HiRISE camera was built by Ball Aerospace and Technology Corporation and is operated by the University of Arizona. The image data were processed using the U.S. Geological Survey’s ISIS3 software.