Explorer I
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| Missing image 0200146.jpg Explorer 1 | |
| Organization: | Army Ballistic Missile Agency |
| Major Contractors: | Jet Propulsion Laboratory |
| Mission Type: | Earth Science |
| Satellite of: | Earth |
| Launch: | February 1, 1958 at 03:48 UTC |
| Launch Vehicle: | Jupiter-C |
| Decay: | March 31, 1970 |
| Mission Duration: | 111 days |
| Mass: | 13.97 kg |
| NSSDC ID: | 1958-001A |
| Webpage: | NASA (http://nssdc.gsfc.nasa.gov/database/MasterCatalog?sc=1958-001A) |
| Orbital elements | |
|---|---|
| Semimajor Axis: | 7,832.2 km |
| Eccentricity: | .139849 |
| Inclination: | 33.24° |
| Orbital Period: | 114.8 minutes |
| Apogee: | 2,550 km |
| Perigee: | 358 km |
| Orbits: | ~56,000 |
| Instruments | |
| Geiger-Mueller detector : | Detection of cosmic rays |
| Wire grid array : | Micrometeorite detection |
| Acoustic detector : | Micrometeorite detection |
Explorer-I, officially known as Satellite 1958 Alpha, was the first United States Earth satellite and was sent aloft as part of the United States program for the International Geophysical Year 1957-1958. It was designed and built by the Jet Propulsion Laboratory (JPL) of the California Institute of Technology under the direction of Dr. William H. Pickering. The satellite instrumentation of Explorer-I was designed and built by Dr. James Van Allen of the State University of Iowa.
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Mission Description
The satellite was launched from Cape Canaveral (now Kennedy Space Center) in Florida at 10:48pm EST on January 31, 1958, by the Jupiter-C vehicle.
The Jupiter-C has its origins in the United States Army's Project Orbiter in 1954. The project was canceled in 1955, however, when the decision was made to proceed with Project Vanguard.
Following the launch of the Soviet Sputnik I on October 4, 1957, ABMA was directed to proceed with the launching of a satellite using the Jupiter-C, which had already been flight-tested in nose-cone re-entry tests for the Jupiter IRBM (intermediate-range ballistic missile). Working closely together, ABMA and JPL completed the job of modifying the Jupiter-C and building the Explorer-I in 84 days.
Spacecraft Design
Explorer I was equipped with a geiger counter for the purposes of detecting cosmic rays. Sometimes the instrumentation would report the expected cosmic-ray count (~30 counts per second) but sometimes it would show a peculiar 0 counts per second. The Iowa group (under Van Allen) noted that all of the 0 counts per second reports were from an altitude of 2000+ km over South America, while passes at 500 km would show the expected level of cosmic rays. After Explorer III, it was decided that the original geiger counter had been overwhelmed by strong radiation coming from a belt of charged particles trapped in space by the Earth's magnetic field. (see: Van Allen radiation belt)
Mission Results
The discovery of the Van Allen Belts by the Explorer satellites was considered to be one of the outstanding discoveries of the International Geophysical Year.
Explorer-I was placed in an orbit with a perigee of 360 kilometers (224 miles) and an apogee of 2520 kilometers (1575 miles) having a period of 114.9 minutes. Its total weight was 13.9 kilograms (30.7 pounds), of which 8.3 kilograms (18.3 pounds) were instrumentation. The instrument section at the front end of the satellite and the empty scaled-down fourth-stage rocket casing orbited as a single unit, spinning around its long axis at 750 revolutions per minute.
Instrumentation consisted of a cosmic-ray detection package, an internal temperature sensor, three external temperature sensors, a nose-cone temperature sensor, a micrometeorite impact microphone, and a ring of micrometeorite erosion gauges. Data from these instruments were transmitted to the ground by a 60-milliwatt transmitter operating on 108.03 megahertz and a 10-milliwatt transmitter operating on 108.00 MHz.
Transmitting antennas consisted of two fibreglass slot antennas in the body of the satellite itself and four flexible whips forming a turnstile antenna. The rotation of the satellite about its long axis kept the flexible whips extended.
The external skin of the instrument section was painted in alternate strips of white and dark green to provide passive temperature control of the satellite. The proportions of the light and dark strips were determined by studies of shadow-sunlight intervals based on firing time, trajectory, orbit, and inclination.
Electrical power was provided by nickel-cadmium chemical batteries that made up approximately 40 percent of the payload weight. These provided power that operated the high power transmitter for 31 days and the low-power transmitter for 105 days.
Because of the limited space available and the requirements for low weight, the Explorer-I instrumentation was designed and built with simplicity and high reliability in mind. It was completely successful.
Explorer I ceased transmission of data on May 23, 1958, when its batteries died, but remained in orbit for more than 12 years. It made a fiery reentry over the Pacific Ocean on March 31, 1970. Explorer I was the first of the long-running Explorer program, which as of March 2000 has launched 78 Explorer probes.
The identically-constructed flight backup of Explorer I is currently located in the Smithsonian Institution's National Air and Space Museum, Milestones of Flight Gallery.
See Also
Reference
- Data Sheet, Department of Astronautics, National Air and Space Museum, Smithsonian Institution.
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