Mariner 9

Mariner Missions

The U.S. exploration of Mars began on November 5 1964 with the launch of Mariner 3. It was an unfortunate beginning to Mars exploration as shortly after launch, a plastic shroud designed to protect the craft failed to separate and the spacecraft went into orbit around the Sun.

Mariner 4 quickly followed on November 28, after an intense project to construct a stronger shroud. This was the first success, and after slight course adjustments, the craft shot past Mars on July 16, 1965. Unfortunately, only 30minutes of pictures could be taken (22 exposures) before Mars disappeared into the distance and Mariner 4 was left to orbit around the Sun. Radio contact has been lost and gained several times since then, and the spacecraft (also carrying many experiments) has sent back some important results. The photographs showed little contrast, but many craters were observed. The Martian surface was consequently compared to that of the Moon. This is now known to be a very unrealistic comparison.

Mariners 6-7 were scheduled for launch in 1969, and the first successfully left for Mars on February 24. Mariner 7 was launched a month later. Both crafts were heavier than their predecessors and carried much more scientific equipment. On August 1, Mariner 6 successfully took 33 pictures of Mars over 20 hours. A second sequence of 25 pictures was taken at close range as the craft travelled around the equatorial region of Mars. Once this was completed, Mariner 6's mission was done. Mariner 7 had a far more eventful journey, and contact was temporarily lost as the craft apparently spun out of control. After long hours, contact was regained and eventually, on August 2, a series of 91 pictures were taken at long range. After reprogramming, a second series of 33 pictures were taken at close range. The images were very misleading, and left astronomers believing that Mars had few if any Earth like forms and did not undergo any of the internal processes that our home planet does. Also, the terrain was seen as almost totally cratered in a similar way to the Moon, and it appeared as though Mars had never had an atmosphere like Earth's. Finally, it was inferred that water did not play any important role in modifying the Martian surface. Today, we know all of these assumptions to be wrong, but many other spacecraft had to travel there before we could see this.

Results from the spectrometer aboard Mariner6-7 proved the previous observations of a CO2 (carbon dioxide) rich atmosphere. However, a number of peaks also suggested the presence of CH4 (methane) and NH3 (ammonia) which, in the Earth's atmosphere, are produced by biological processes. This was probably the strongest indication of life on Mars ever seen, and it sparked off much excitement.

Mariner 4
Mariner 6/7

Mariner 9 was the first major Mars mission, arriving at the planet on November 13 1971, after a journey of 400 million km. Upon arrival, Mars was enveloped in a global dust storm which settled only after a few weeks. Mariner 9 was then able to show us Mars as it was never seen before. The largest volcanoes in the solar system were observed to protrude from the Martian cloud cover, dwarfing the Earth's largest offerings. The largest volcano, Olympus Mons, rises more than 24 km (15 miles) from the Martian surface (almost three times as high as Mt. Everest on Earth) and was formed by `hotspot' activity, similar to the Hawai'ian Islands on Earth. The Hawai'ian Islands are also affected by plate tectonics, with different regions gradually moving over the active area, so volcanoes do not remain active for the whole life of the hotspot. The shear size of Olympus Mons suggests that it probably remained over the hotspot for its whole life, which in turn is suggestive of the absence of plate tectonics on Mars.
Comparison of the sizes of Olympus Mons and Mt. Everest

Olympus Mons covers an area equivalent in size to the state of Missouri (about half of Spain) and is located in the Northern hemisphere close to a band of three large volcanoes on a raised plateau called Tharsis Ridge. This area is about 5 to 6 km higher than the average ground level on Mars and forms part of the famous `Martian Dichotomy' whereby most of the craters on Mars are located in the Southern hemisphere, while the plains and volcanoes are to the North. Mariner 9 also observed Valles Marineris, a vast canyon region running roughly parallel to the Martian equator and stretching some 300 km across the surface (equivalent to the distance between Los Angeles and New York on Earth). This penetrates some 8 km down from the plateau and is thought to be the result of internal stresses on Mars (possibly similar to rift valleys on Earth). Other features on Mars are remarkably similar to dried up river beds on Earth and may indicate the flow of water across the surface of ancient Mars, although modern theories also suggest they may result from water below the surface in a process called `sapping'.
Olympus Mons