Courtesy of NASA's National Space Science Data Center
NASA's Viking Mission to Mars was composed of two spacecraft, Viking 1 and Viking 2. Each spacecraft consisted of an orbiter and a lander. The primary mission objectives were to
The Viking Landers transmitted images of the surface, took surface samples and analyzed them for composition and signs of life, studied atmospheric composition and meteorology, and deployed seismometers. Viking Lander 2 ended communications on April 11, 1980, and Viking Lander 1 on November 13, 1982, after transmitting over 1400 images of the two sites.
The results from the Viking experiments give our most complete view of Mars to date. Volcanoes, lava plains, immense canyons, cratered areas, wind-formed features, and evidence of surface water are apparent in the orbiter images. The planet appears to be divisible into two main regions, northern low plains and southern cratered highlands. Superimposed on these regions are the Tharsis and Elysium bulges, which are high-standing volcanic areas, and Valles Marineris, a system of giant canyons near the equator. The surface material at both landing sites can best be characterized as iron-rich clay. Measured temperatures at the landing sites ranged from 150 to 250 Kelvin, with a variation over a given day of 35 to 50 Kelvin. Seasonal dust storms, pressure changes, and transport of atmospheric gases between the polar caps were observed. The biology experiment produced no evidence of life at either landing site.
Viking Mission to Mars
The Viking mission to Mars sent twin spacecraft to the Red Planet. This image shows a model of one of the Viking spacecraft, which were made of two parts: an orbiter and a lander. The orbiter's initial job was to survey the planet for a suitable landing site. Later the orbiter's instruments studied the planet and its atmosphere, while the orbiter acted as a radio relay station for transmitting lander data. Once on the surface of Mars, the lander surveyed the soil, wind, and atmosphere and conducted numerous experiments to determine the existence of past or present life. (Courtesy NASA/JPL)
In this artist's rendering a Viking lander released its parachute just after entering the Martian atmosphere. When the parachute was deployed, the lander pod was at an altitude of about 6 kilometers (4.0 miles) and traveling at a velocity of 900 kilometers per hour (600 mph). Soon after, the lower half of the heat shield fell away and the lander's legs unfolded. At an altitude of about 1.5 kilometers (5,000 feet) the pod separated from the parachute and using three retro-engines to control its descent, landed safely on the surface of Mars. (Courtesy NASA/JPL)
Captured here in this rendering is a Viking lander just before it touched down on the Martian surface. The parachute and upper aeroshell can be seen in the upper left corner of the image. At this stage of the descent, the lander's terminal descent propulsion system (three retro-engines) had slowed the craft down so that velocity at landing was about of 2 meters per second (7 mph). Seconds after the lander reached the surface it began transmitting images back to the orbiter for relay to Earth. (Courtesy NASA/JPL)
Viking On the Surface of Mars
This photograph shows a model of the Viking lander on a simulated Martian surface. The first of the two landers arrived on the surface of Mars on July 20, 1976. The second touched down on September 3, 1976. Each lander housed instruments that examined the physical and magnetic properties of the soil and analyzed the atmosphere and weather patterns of Mars. (Courtesy NASA/JPL)