Ranger 2
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|
Mission type | Technology |
---|---|
Operator | NASA |
Harvard designation | 1961 Alpha Theta 1 |
COSPAR ID | 1961-032A |
SATCAT no. | 206 |
Mission duration | 2 days |
Spacecraft properties | |
Manufacturer | Jet Propulsion Laboratory |
Launch mass | 304 kilograms (670 lb) |
Power | 150 W |
Start of mission | |
Launch date | 18 November 1961, 08:09:00 | UTC
Rocket | Atlas LV-3 Agena-B |
Launch site | Cape Canaveral LC-12 |
End of mission | |
Decay date | 20 November 1961 |
Orbital parameters | |
Reference system | Geocentric |
Regime |
Low Earth (High Earth planned) |
Semi-major axis | 6,574.2 kilometres (4,085.0 mi) |
Perigee | 150 kilometres (93 mi) |
Apogee | 242 kilometres (150 mi) |
Inclination | 33.3 degrees |
Period | ~89 minutes |
Instruments | |
Lyman-Alpha Telescope Magnetometer |
Ranger 2 was a flight test of the Ranger spacecraft system of the NASA Ranger program designed for future lunar and interplanetary missions. Ranger 2 was designed to test various systems for future exploration and to conduct scientific observations of cosmic rays, magnetic fields, radiation, dust particles, and a possible hydrogen gas "tail" trailing the Earth.
Ranger 2 was of the Ranger Block 1 design and was almost identical to Ranger 1. The spacecraft consisted of a hexagonal base 1.5 m across, upon which was mounted a cone-shaped 4-meter-high tower of aluminum struts and braces. Two solar panel wings measuring 5.2 m from tip to tip extended from the base. A high-gain directional dish antenna was attached to the bottom of the base. Spacecraft experiments and other equipment were mounted on the base and tower. Instruments aboard the spacecraft included a Lyman-alpha telescope, a rubidium-vapor magnetometer, electrostatic analyzers, medium-energy-range particle detectors, two triple coincidence telescopes, a cosmic-ray integrating ionization chamber, cosmic dust detectors, and scintillation counters.
The communications system included the high-gain antenna and an omnidirectional medium-gain antenna and two transmitters at approximately 960 MHz, one with 0.25 W power output and the other with 3 W power output. Power was to be furnished by 8680 solar cells on the two panels, a 53.5 kg silver-zinc battery, and smaller batteries on some of the experiments. Attitude control was provided by a solid state timing controller, Sun and Earth sensors, gyroscopes, and pitch and roll jets. The temperature was controlled passively by gold plating, white paint, and polished aluminum surfaces.