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1 Design and instruments  





2 Mission  





3 Communications  





4 See also  





5 References  





6 External links  














Pioneer 5






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Pioneer 5
Pioneer 5 mounted to its Thor Able launcher.
Mission typeInterplanetary space research
OperatorNASA
Harvard designation1960 Alpha 1
COSPAR ID1960-001A Edit this at Wikidata
SATCAT no.27
Mission durationLaunch to last contact 107 days; launch to last data received 50 days
Spacecraft properties
ManufacturerTRW
Launch mass43.2 kilograms (95 lb)[1]
Start of mission
Launch date11 March 1960, 13:00:07 UTC (1960-03-11UTC13:00:07)
RocketThor DM 18-Able IV
Launch siteCape Canaveral, LC-17A
ContractorDouglas
End of mission
Last contactLast contact 26 June 1960 (1960-06-27);[1] last data received 30 April 1960[2]
Orbital parameters
Reference systemHeliocentric
Eccentricity0.1689
Perihelion altitude0.7061 astronomical units (105,630,000 km; 65,640,000 mi)
Aphelion altitude0.9931 astronomical units (148,570,000 km; 92,310,000 mi)
Inclination3.35°
Period311.6 days
 

Pioneer 5 (also known as Pioneer P-2, and Able 4, and nicknamed the "Paddle-Wheel Satellite"[3]) was a spin-stabilized space probe in the NASA Pioneer program used to investigate interplanetary space between the orbits of Earth and Venus. It was launched on 11 March 1960 from Cape Canaveral Air Force Station Launch Complex 17A at 13:00:00 UTC[4] with an on-orbit dry mass of 43 kilograms (95 lb). It was a 0.66 metres (2 ft 2 in) diameter sphere with 1.4 metres (4 ft 7 in) span across its four solar panels and achieved a solar orbit of 0.806 × 0.995 AU (121,000,000 by 149,000,000 km).

Data was received until 30 April 1960. Among other accomplishments, the probe confirmed the existence of interplanetary magnetic fields.[5] Pioneer 5 was the most successful probe in the Pioneer/Able series.

The original mission plan was for a launch in November 1959 where Pioneer 5 would conduct a flyby of Venus, but technical issues prevented the launch from occurring until early 1960 by which time the Venus window for the year had closed. Since it was not possible to send the probe to Venus, it would instead merely investigate interplanetary space and an actual mission to the planet would have to wait another three years.[6]

Design and instruments[edit]

The spacecraft was a 0.66 metres (2 ft 2 in) diameter sphere with four solar panels that spanned over 1.4 metres (4 ft 7 in) and it was equipped with four scientific instruments:

  1. Atriple coincidence omnidirectional proportional counter telescope to detect solar particles and observe terrestrial trapped radiation. It could detect photons with E >75MeV and electrons with E > 13 MeV.[7]
  2. Arotating search coil magnetometer to measure the magnetic field in the distant field of the Earth, near the geomagnetic boundary, and in interplanetary space.[8][9] It was capable of measuring fields from 1 microgauss to 12 milligauss. It consisted of a single search coil that was mounted on the spacecraft in such a way that it measured the magnetic field perpendicular to the spin axis of the spacecraft. It could output its measurements in both an analog and a digital format.[10]
  3. ANeher-type integrating ionization chamber and an Anton 302 Geiger-Müller tube (which functioned as a cosmic ray detector) to measure cosmic radiation. It was mounted normal to the spin axis of the spacecraft.[11]
  4. Amicrometeorite momentum spectrometer (or micrometeorite detector) that consisted of two diaphragm and microphone combinations. It was used to measure the amount of meteoritic dust particles and the momentum of these particles.[12]

Mission[edit]

Booster performance during launch was overall excellent considering the numerous earlier difficulties with the Thor-Able vehicle. There were some minor anomalies with the second stage flight control system that resulted in unplanned pitch and roll motions, however, they were not enough to endanger the mission.

The spacecraft returned data collected by the magnetometer on the magnetic field and it measured that the median undisturbed interplanetary field was approximately 5 γ ± 0.5 γ in magnitude.[13] The spacecraft also measured solar flare particles, and cosmic radiation in the interplanetary region. The micrometeorite counter failed to operate as the data system saturated and failed to operate properly.[12]

Pioneer 5 with test equipment.

The recorded digital data were transmitted at 1, 8, and 64 bit/s, depending on the distance of the spacecraft from Earth and the size of the receiving antenna. Weight limitations on the solar cells prevented continuous operation of the telemetry transmitters. About four operations of 25 min duration were scheduled per day with occasional increases during times of special interest. A total of 138.9 h of operation was completed, and over three megabits of data were received. The major portion of the data was received by the Lovell radio telescopeatJodrell Bank Observatory and the Hawaii Tracking Station because their antennas provided grid reception. Data was received until 30 April 1960, after which telemetry noise and weak signal strength made data reception impossible. The spacecraft's signal was detected by Jodrell Bank from a record distance of 36.2 million km (22.5 million miles) on 26 June 1960, although it was much too weak by then to acquire data.[2]

Communications[edit]

In common with Explorer 6, Pioneer 5 used the earliest known digital telemetry system used on spacecraft, codenamed "Telebit",[14] which was a tenfold (or 10 dB) [14] improvement in channel efficiency on previous generation "Microlock" analog systems in use since Explorer 1 and the biggest single improvement in signal encoding on western spacecraft. The spacecraft received the uplink carrier at 401.8 MHz and converted it to a 378.2 MHz signal using a 16/17 coherent oscillator circuit.[15] The telemetry system phase modulated a 512 Hz subcarrier, which was in turn amplitude modulated at 64, 8, or 1bit/s. The spacecraft was unable to aim its antennas, and so had no high-gain dish antenna common on later spacecraft. Instead, the system could introduce a 150W amplifier into its normally 5W transmitter circuit. It was powered by a battery of 28 F-size NiCd cells recharged by the solar paddles, allowing up to eight minutes of high power communications before risking damage to the batteries.[16] Each hour of 5W communications or five minutes of 150W communications required ten hours of recharging the batteries. Unlike later interplanetary spacecraft (Mariner 2 and beyond), this spacecraft did not use the Deep Space Network, which was not yet available, but a somewhat ad hoc Space Network called SPAN consisting of the 76m Lovell Telescope (then called Manchester Mark I), a 26-meter radio telescope in Hawaii, and a small helical array in Singapore.

See also[edit]

References[edit]

  1. ^ a b "Pioneer 5 - NASA Science". science.nasa.gov. NASA. Retrieved 1 December 2022.
  • ^ a b "Pioneer 5". nssdc.gsfc.nasa.gov. NASA. Retrieved 31 January 2008.
  • ^ Patrick Moore (1962). The Observer's Book of Astronomy. Frederick Warne & Co.
  • ^ Mark Wade. "1960 Chronology". Encyclopedia Astronautica. Retrieved 31 January 2008.
  • ^ "The Pioneer Spacecraft". NASAFacts. NF-31/Vol 4, No. 3. U.S. Government Printing Office, 1967.
  • ^ Andrew LePage (17 April 2015). "Vintage Micro: The First Interplanetary Probe". www.drewexmachina.com.
  • ^ "Pioneer 5: Proportional Counter Telescope". nssdc.gsfc.nasa.gov. NASA. Retrieved 31 January 2008.
  • ^ P. J. Coleman; L. Davis; C. P. Sonett (15 July 1960). "Steady Component of the Interplanetary Magnetic Field: Pioneer V". Physical Review Letters. 5 (2): 43–46. Bibcode:1960PhRvL...5...43C. doi:10.1103/PhysRevLett.5.43.
  • ^ J. W. Dungey (15 January 1961). "Interplanetary Magnetic Field and the Auroral Zones". Physical Review Letters. 6 (2): 47–48. Bibcode:1961PhRvL...6...47D. doi:10.1103/PhysRevLett.6.47. Archived from the original on 24 September 2017.
  • ^ "Pioneer 5: Search-Coil Magnetometer". nssdc.gsfc.nasa.gov. NASA. Retrieved 31 January 2008.
  • ^ "Pioneer 5: Ion Chamber and GM Tube". nssdc.gsfc.nasa.gov. NASA. Retrieved 31 January 2008.
  • ^ a b "Pioneer 5: Micrometeorite Spectrometer". nssdc.gsfc.nasa.gov. NASA. Retrieved 31 January 2008.
  • ^ E. W. Greenstadt (July 1966). "Final Estimate of the Interplanetary Magnetic Field at 1 A.U. from Measurements made by Pioneer V in March and April 1960". Astrophysical Journal. 145 (1): 270–295. Bibcode:1966ApJ...145..270G. doi:10.1086/148761.
  • ^ a b G. E. Miller; J. E. Taber (1959). An Interplanetary Communication System abstract (PDF). STL/TR. Retrieved 6 August 2015.
  • ^ A. Good (1 June 1960). Payload Command Receiver/Doppler Transponder (PDF). STL/TR. Retrieved 6 August 2015.
  • ^ Project Thor-Able 4 Final Mission Report (PDF). STL/TR. 25 May 1960. pp. 4–25. Retrieved 6 August 2015.
  • External links[edit]


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