Mariner 2

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Mariner 2
Mariner 2.jpg
Depiction of Mariner 2 in space
Mission type Planetary flyby
Operator NASA / JPL
Harvard designation 1962 Alpha Rho 1[1]
COSPAR ID 1962-041A
SATCAT no. 374
Mission duration 4 months, 7 days
Spacecraft properties
Spacecraft type Mariner
based on Ranger Block I
Manufacturer Jet Propulsion Laboratory
Launch mass 202.8 kilograms (447 lb)
Power 220 watts (at Venus encounter)
Start of mission
Launch date August 27, 1962, 06:53:14 (1962-08-27UTC06:53:14Z) UTC[1]
Rocket Atlas LV-3 Agena-B
Launch site Cape Canaveral LC-12
End of mission
Last contact January 3, 1963 (1963-01-04)
Orbital parameters
Reference system Heliocentric
Perihelion 105,464,560 kilometers (56,946,310 nautical miles)
Epoch December 27, 1962
Flyby of Venus
Closest approach December 14, 1962
Distance 34,773 kilometers (18,776 nautical miles)

Mariner 2 was a NASA spacecraft. It was the second spacecraft in the Mariner program. Mariner 2 was the first successful mission from Earth to another planet.

Mission[change | change source]

Mariner 2 was launched on August 27, 1962 aboard an Atlas-Agena B rocket at Cape Canaveral Air Force Station. The aim of the Mariner 2 mission was to fly-by the planet Venus and return information on the planet's atmosphere, magnetic field, charged particle environment, and mass. Mariner 2 was at its closest to Venus, at a distance of 34,773 km, on December 14, 1962. The spacecraft then went into orbit with the Sun on Sepember 27, 1962, 105,464,560 km away. The last transmission from Mariner 2 was received on January 3, 1963. Mariner 2 is still orbiting around the Sun today.

Design[change | change source]

The spacecraft's design was exactly the same as that of Mariner 1. Mariner 1 was the first spacecraft in the Mariner program, but it had to be destroyed shortly after launch because its trajectory was wrong.

Discoveries[change | change source]

The spacecraft found out that the surface temperature on Venus was at least 425 °C (797 °F), on both the day and night sides. It discovered that Venus rotates in the opposite direction from most planets in the Solar System. The spacecraft also found that the atmosphere of Venus is mostly of carbon dioxide and that there is a very high pressure at the planet's surface. Continuous cloud cover was detected but no magnetic field was, however. It also found that solar wind is continuous and that the density of cosmic dust between planets is much lower than it is near Earth.

References[change | change source]

  1. 1.0 1.1 McDowell, Jonathan. "Launch Log". Jonathan's Space Page. Retrieved 12 September 2013. 

Other websites[change | change source]