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Ranger 2
Organization: NASA
Major Contractors: Jet Propulsion Laboratory
Mission Type: Lunar Science
Satellite of: Earth
Launch: November 18, 1961 at 08:09:00 UTC
Launch Vehicle: Atlas-Agena B
Decay: November 20, 1961
Mission Duration: 2 days
Mass: 304 kg
NSSDC ID: 1961-032A
Webpage: NASA NSSDC Master Catalog
Orbital elements
Semimajor Axis: 6,574.2 km
Eccentricity: .?
Inclination: 33.3°
Orbital Period:~89 minutes
Apogee: 242 km
Perigee: 150 km
Orbits: 32
Instruments
Lyman-Alpha Telescope : scan earth to study hydrogen constituent of exosphere
Magnetometer : Measure magnetic field in interplanetary space


Ranger 2 was a flight test of the Ranger spacecraft system of the 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.

1 Spacecraft design

Ranger 2 was of the Ranger Block 1 design and was almost identical to Ranger 1Ranger 1 was a spacecraft in the Ranger program whose primary mission was to test the performance of those functions and parts necessary for carrying out subsequent lunar and planetary missions. A secondary objective was to study the nature of particles a. The spacecraft consisted of a hexagonal base 1.5 m across upon which was mounted a cone-shaped 4 m 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 magnetometerA Magnetometer is a scientific instrument used to measure the strength of magnetic fields. Earth's magnetism varies from place to place and differences in the Earth's magnetic field (the magnetosphere) can be caused by a couple of things: #The differing n, electrostatic analyzers, medium-energy-range particle detectors, two triple coincidence telescopes, a cosmic-ray integrating ionization chamber, cosmic dust detectors, and scintillation counterA scintillation counter measures ionizing radiation. The sensor, called a scintillator, consists of a transparent crystal, plastic (usually containing anthracene), or organic liquid (see liquid scintillation counting) that fluoresces when struck by ionizis.

The communications system included the high gain antenna and an omni-directional 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, SunThe Sun (also called Sol is the star in our solar system. Planet Earth orbits the Sun. Other bodies that orbit the Sun include other planets, asteroids, meteoroids, comets and dust. Not all objects passing through the solar system have been orbitally capt and Earth sensors, gyroscopes, and pitch and roll jets. The temperature was controlled passively by gold plating, white paint, and polished aluminum surfaces.



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