SYRTIS MAJOR

Mars, with Syrtis Major visible in the planet's centre. Image taken by the Mars Global Surveyor on Syrtis Major region on Mars. This enhanced-colour mosaic, which combines images taken by the Viking distinctive dark marking on the surface of the planet Mars, centred near 290 W and 10 N, which extends some 1,500 km (930 miles) north from the planet's equator and spans 1,000 km (620 miles) from west to east. It was noticed as early as 1659, for it appears in a drawing of Mars of that date by Christiaan Huygens. It is an extensive regional slope elongated north to south that drops 4 km (2.5 miles) from its western boundary (Aeria) to its eastern edge (Isidis). Assiduously observed for more than a century because of its seasonal and long-term variability, especially near its eastern boundary, Syrtis Major was first considered a shallow sea. Later its variability was attributed to vegetation. Closeup photographs and data returned by the U.S. Mariner and Viking planetary probes during the 1960s and '70s enabled investigators to determine that the changes are caused by wind blowing sand and dust across the surface. In the early 1980s detailed topographical maps, prepared from Earth-based spectroscopic and radar observations as well as from the space-probe photographs, indicated that Syrtis Major includes a high-altitude bulge rising to 6 km (3.7 miles) at 310 W.