Mariner 9

Mariner 9

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Mariner 9

Mariner 9 (Mariner Mars '71 / Mariner-I) was a NASA space probe orbiter that helped in the exploration of Mars and was part of the Mariner program. Mariner 9 was launched toward Mars on May 30, 1971 from Cape Canaveral Air Force Station and reached the planet on November 13 of the same year, becoming the first spacecraft to orbit another planet ? only narrowly beating Soviet Mars 2 and Mars 3, which both arrived within a month. After months of dust-storms it managed to send back surprisingly clear pictures of the surface.

Objectives
Instruments
Achievements
Construction
Present location
See also
External links

Objectives

Mariner 9 launch

Mariner 9 was designed to continue the atmospheric studies begun by Mariner 6 and 7, and to map over 70% of the Martian surface from the lowest altitude (1500 kilometers [about 900 miles]) and at the highest resolutions (1 kilometer per pixel to 100 meters per pixel) of any Mars mission up to that time. An infrared radiometer was included to detect heat sources as evidence of volcanic activity. It was to study temporal changes in the Martian atmosphere and surface. Mars' two moons were also to be analyzed. Mariner 9 more than met its objectives.

Instruments

Ultraviolet Spectrometer (UVS)
Infrared Interferometer Spectrometer (IRIS)
Celestial Mechanics
S-Band Occultation
Infrared Radiometer (IRR)
Television Photography

Achievements

Mariner 9 view of the Noctis Labyrinthus "labyrinth" at the western end of Valles Marineris.

Mariner 9 was the first spacecraft to orbit another planet. It carried an instrument payload similar to Mariner 6 and 7, but, because of the need for a larger propulsion system to control the spacecraft in Mars orbit, it weighed more than Mariners 6 and 7 combined. When Mariner 9 arrived at Mars, the atmosphere was so dusty that the surface was obscured. This unexpected situation made a strong case for the desirability of studying a planet from orbit rather than merely flying past. Mariner 9's computer was thus programmed from Earth to delay imaging of the surface for a couple of months until the dust settled. After 349 days in orbit, Mariner 9 had transmitted 7,329 images, covering over 80% of Mars' surface. The images revealed river beds, craters, massive extinct volcanoes (such as Olympus Mons, the largest known volcano in the Solar System), canyons (including the Valles Marineris, a system of canyons over about long), evidence of wind and water erosion and deposition, weather fronts, fogs, and more. Mars' tiny moons, Phobos and Deimos, were also photographed. The findings from the Mariner 9 missions underpinned the later Viking program.

The enormous Valles Marineris canyon system is named after Mariner 9 in honour of its achievements.

After depleting its supply of attitude control gas, the spacecraft was turned off on 27 October, 1972.

Construction

The ultraviolet spectrometer aboard Mariner 9 was constructed by the Laboratory for Atmospheric and Space Physics.

Present location

Mariner 9 is still in Mars orbit, stable until at least 2022, after which the spacecraft will enter the Martian atmosphere.

External links

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Mariner 9

Contents

Objectives

Instruments

Achievements

Construction

Present location

See also

External links