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Mariner 10

Mariner 10
File:Mariner 10 gravitational slingshot.jpg
Artist's impression of the Mariner 10 mission
Mission type Planetary exploration
Operator NASA / JPL
COSPAR ID 1973-085A[1]
SATCAT № 6919[1]
Mission duration 1 year, 4 months, 12 days
Spacecraft properties
Manufacturer Jet Propulsion Laboratory
Launch mass Script error: No such module "convert".
Power 820 watts (at Venus encounter)
Start of mission
Launch date November 3, 1973, 05:45:00 (1973-11-03UTC05:45Z) UTC
Rocket Atlas SLV-3D Centaur-D1A
Launch site Cape Canaveral LC-36B
End of mission
Disposal Decommissioned
Deactivated March 24, 1975 (1975-03-25)

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Mariner 10 was an American robotic space probe launched by NASA on November 3, 1973, to fly by the planets Mercury and Venus.

Mariner 10 was launched approximately two years after Mariner 9 and was the last spacecraft in the Mariner program (Mariner 11 and 12 were allocated to the Voyager program and redesignated Voyager 1 and Voyager 2).

The mission objectives were to measure Mercury's environment, atmosphere, surface, and body characteristics and to make similar investigations of Venus. Secondary objectives were to perform experiments in the interplanetary medium and to obtain experience with a dual-planet gravity assist mission. Mariner 10's science team was led by Bruce C. Murray at the Jet Propulsion Laboratory.[2]

Design and trajectory

Mariner 10 was the first spacecraft to make use of an interplanetary gravitational slingshot maneuver, using Venus to bend its flight path and bring its perihelion down to the level of Mercury's orbit.[3] This maneuver, inspired by the orbital mechanics calculations of the Italian scientist Giuseppe Colombo, put the spacecraft into an orbit that repeatedly brought it back to Mercury. Mariner 10 used the solar radiation pressure on its solar panels and its high-gain antenna as a means of attitude control during flight, the first spacecraft to use active solar pressure control. The Mariner 10 spacecraft was manufactured by Boeing.[4]


An illustration showing Mariner 10's instruments

Mariner 10 instruments included:

  1. Twin telescope/cameras with digital tape recorder
  2. Ultraviolet spectrometer
  3. Infrared radiometer
  4. Solar plasma
  5. Charged particles
  6. Magnetic fields
  7. Radio occultation
  8. Celestial mechanics

The imaging system, the Television Photography Experiment, consisted of two 15 cm (5.9″) Cassegrain telescopes feeding vidicon tubes.[5] The entire imaging system was imperiled when electric heaters attached to the cameras failed to turn on immediately after launch. The cameras were deliberately placed on the spacecraft side facing away from the Sun so as to avoid the Sun's damaging heat, but consequently the heaters were needed to prevent the extremely cold environment from harming the cameras. JPL engineers found that the vidicons could generate enough heat through normal operation to stay just above the critical temperature of -40°C; therefore they advised against turning off the cameras during the flight. Fortunately, test photos of the Earth and Moon showed that image quality had not been significantly affected.[6] The camera heaters started working for the first time on January 17, two months after launch. Later investigation concluded that a short circuit in a different location on the probe had prevented the heater from turning on. This allowed the vidicons to be turned off as needed.[7][8][9] The main telescope could be bypassed to a smaller wide angle optic, but using the same tube.[5] It had an 8-position filter wheel, with one position occupied by a mirror for the wide-angle bypass.[5] The system returned about 7000 photographs of Mercury and Venus during Mariner 10's flybys.[5]

Departing the Earth–Moon system

File:Mariner-10-Trajectory-first half.PNG
Trajectory of Mariner 10 spacecraft: since launch on November 3, 1973, to first fly-by of Mercury on March 29, 1974
File:Mariner 10.jpg
The Mariner 10 probe, the first probe to visit Mercury

During its first week of flight, Mariner 10 tested its camera system by returning five photographic mosaics of Earth and six of the Moon. It also obtained photographs of the north polar region of the moon where prior coverage was poor. These provided a basis for cartographers to update lunar maps and improve the lunar control net.[10]

Cruise to Venus

A trajectory correction maneuver was made on November 13, 1973. Immediately afterwards, the star-tracker locked onto a bright flake of paint which had come off the spacecraft and lost tracking on the guide star Canopus. An automated safety protocol recovered Canopus, but the problem of flaking paint recurred throughout the mission. The on-board computer also experienced unscheduled resets occasionally, which necessitated reconfiguring the clock sequence and subsystems. Periodic problems with the high-gain antenna also occurred during the cruise. In January 1974, Mariner 10 made ultraviolet observations of Comet Kohoutek. Another mid-course correction was made on January 21, 1974.

Venus flyby

The spacecraft passed Venus on February 5, 1974, the closest approach being 5,768 km at 17:01 UT. Using a near-ultraviolet filter, it photographed Venus's chevron clouds and performed other atmospheric studies. It was discovered that extensive cloud detail could be seen through Mariner's ultraviolet camera filters. Venus's cloud cover is nearly featureless in visible light. Earth-based ultra-violet observation did reveal some indistinct blotching even before Mariner 10, but the detail seen by Mariner was a surprise to most researchers.

First Mercury flyby

The first Mercury encounter took place at 20:47 UT on March 29, 1974, at a range of Script error: No such module "convert"., passing on the shadow side.[3]

Second Mercury flyby

After looping once around the Sun while Mercury completed two orbits, Mariner 10 flew by Mercury again on September 21, 1974, at a more distant range of Script error: No such module "convert". below the southern hemisphere.[3]

Third Mercury flyby

After losing roll control in October 1974, a third and final encounter, the closest to Mercury, took place on March 16, 1975, at a range of Script error: No such module "convert"., passing almost over the north pole.[3]

End of mission

With its maneuvering gas just about exhausted, Mariner 10 started another orbit of the Sun. Engineering tests were continued until March 24, 1975,[3] when final depletion of the nitrogen supply was signaled by the onset of an un-programmed pitch turn. Commands were sent immediately to the spacecraft to turn off its transmitter, and radio signals to Earth ceased.

Mariner 10 is still orbiting the Sun, although its electronics have probably been damaged by the Sun's radiation.[11] Dave Williams of NASA's National Space Science Data Center said in 2005: "Mariner 10 has not been tracked or spotted from Earth since it stopped transmitting. We can only assume it's still orbiting [the Sun], but the only way it would not be orbiting would be if it had been hit by an asteroid or gravitationally perturbed by a close encounter with a large body. The odds of that happening are extremely small, so it is assumed to still be in orbit."


During its flyby of Venus, Mariner 10 discovered evidence of rotating clouds and a very weak magnetic field.

The spacecraft flew past Mercury three times. Owing to the geometry of its orbit – its orbital period was almost exactly twice Mercury's – the same side of Mercury was sunlit each time, so it was only able to map 40–45% of Mercury’s surface, taking over 2,800 photos. It revealed a more or less Moon-like surface. It thus contributed enormously to our understanding of Mercury, whose surface had not been successfully resolved through telescopic observation. The regions mapped included most or all of the Shakespeare, Beethoven, Kuiper, Michelangelo, Tolstoj, and Discovery quadrangles, half of Bach and Victoria quadrangles, and small portions of Solitudo Persephones (later Neruda), Liguria (later Raditladi), and Borealis quadrangles.[12]

Mariner 10 also discovered that Mercury has a tenuous atmosphere consisting primarily of helium, as well as a magnetic field and a large iron-rich core. Its radiometer readings suggested that Mercury has a night time temperature of −183 °C (−297 °F) and maximum daytime temperatures of 187 °C (369 °F).

Planning for MESSENGER, a spacecraft that surveyed Mercury until 2015, relied extensively on data and information collected by Mariner 10.

Mariner 10 Commemoration

On February 10, 1975, the US Post Office issued a commemorative stamp featuring the Mariner 10 space probe. The 10-cent Mariner 10 commemorative stamp was issued on April 4, 1975, at Pasadena, California.

See also



  1. ^ a b "Mariner 10". US National Space Science Data Center. Retrieved 7 September 2013. 
  2. ^ Schudel, Matt (30 August 2013). "Bruce C. Murray, NASA space scientist, dies at 81". The Washington Post. Retrieved 31 August 2013. 
  3. ^ a b c d e "Mariner 10". Retrieved 2 February 2014. 
  4. ^ "Mariner 10 Quicklook". Retrieved 31 July 2014. 
  5. ^ a b c d NASA/NSSDC – Mariner 10 – Television Photography
  6. ^ Murray and Burgess 1977, pp. 43–48
  7. ^ Clark, Pamela, ed. (December 2003). "Mariner 10: A Retrospective" (PDF). Mercury Messenger (Lunar and Planetary Institute) (10). Retrieved 25 May 2015. 
  8. ^ Dunne and Burgess 1978, pp. 57–58
  9. ^ "Bulletin No. 14: TCM-2 Performance Superb TV Heaters Have Come On" (PDF). Mariner Venus/Mercury 1973 Project Office. 23 January 1974. Retrieved 25 May 2015. 
  10. ^ Dunne and Burgess 1978, pp. 47–53.
  11. ^ Mariner 10 (2006) Views of the Solar System
  12. ^ Schaber, Gerald G.; McCauley, John F. Geologic Map of the Tolstoj (H-8) Quadrangle of Mercury (PDF). U.S. Geological Survey. USGS Miscellaneous Investigations Series Map I–1199, as part of the Atlas of Mercury, 1:5,000,000 Geologic Series. Retrieved 12 November 2007. 

Further reading

External links

de:Mariner#Mariner 10