PIA00929: MGS Approach Image - 172.4° W Longitude
 Target Name:  Mars
 Is a satellite of:  Sol (our sun)
 Mission:  Mars Global Surveyor (MGS)
 Spacecraft:  Mars Global Surveyor Orbiter
 Instrument:  Mars Orbiter Camera (MOC)
 Product Size:  512 x 512 pixels (w x h)
 Produced By:  Malin Space Science Systems
 Producer ID:  MOC2-5 MRPS84032
 Addition Date:  1997-09-10
 Primary Data Set:  MGS EDRs
 Full-Res TIFF:  PIA00929.tif (42.96 kB)
 Full-Res JPEG:  PIA00929.jpg (8.111 kB)

Click on the image above to download a moderately sized image in JPEG format (possibly reduced in size from original)

Original Caption Released with Image:

This image is the first of a sequence of Mars to be taken by the Mars Global Surveyor Orbiter Camera (MOC) between August 19 and August 21, 1997. It was acquired early in the morning of August 19 when the MGS spacecraft was 5.8 million kilometers (3.6 million miles) and 24 days from encounter. At this distance, the MOC's resolution is about 21.8 km per picture element, and the 6800 km (4200 mile) diameter planet is about 312 pixels across. The MGS spacecraft pointed the camera at the center of the planet (near the dark, morning sunrise line, or terminator) at 23.6° N, 172.4° W. The image shows Olympus Mons, 25 km (15.5 mile) high, 550 km (340 mile) wide volcano, towards the center of the illuminated portion of the planet, with the three other large Tharsis volcanos appearing as dark spots closer to the bright edge, or limb of the planet. The "bulls-eye" appearance of Olympus Mons is likely the result of the interplay between light-colored dust, dark rock, and clouds and fog. The central spot is the light, dust-covered floor of the summit crater (called the caldera), the dark zone is the rocky, less dust-covered upper slope of the volcano, and the outer bright ring is the lower, dust, fog, and cloud covered lower slopes of the volcano. A faint indication of the 3 km high escarpment that surrounds the base of Olympus Mons can be seen as a thin dark line on the outer edge of the bright outer zone. Many of the wispy light areas seen throughout this image are probably other clouds and morning hazes, which have been prominently seen in Hubble Space Telescope images taken this year. The north polar residual ice cap, surrounded by a dark annulus of sand, is seen at the top of this picture.

Malin Space Science Systems and the California Institute of Technology built the MOC using spare hardware from the Mars Observer mission. MSSS operates the camera from its facilities in San Diego, CA. The Jet Propulsion Laboratory operates the Mars Global Surveyor spacecraft with its industrial partner, Lockheed Martin Astronautics, from facilities in Pasadena, CA and Denver, CO.

Image Credit:
NASA/JPL/Malin Space Science Systems

Image Addition Date:
1997-09-10