![]() Artist's impression of Pioneer 12 in orbit above Venus | |
Names | Pioneer Venus 1 Pioneer 12 |
---|---|
Mission type | Venus orbiter |
Operator | NASA / Ames |
COSPAR ID | 1978-051A |
SATCAT no. | 10911 |
Website | science.nasa.gov |
Mission duration | 14 years, 4 months, 18 days (from launch) 13 years, 10 months, 4 days (at Venus) |
Spacecraft properties | |
Bus | HS-507 |
Manufacturer | Hughes |
Launch mass | 582 kg (1,283 lb) [1] |
Dry mass | 517 kg (1,140 lb) |
Dimensions | 2.5 × 1.2 m (8.2 × 3.9 ft) |
Power | 312 watts |
Start of mission | |
Launch date | May 20, 1978, 13:13:00[1] | UTC
Rocket | Atlas SLV-3D Centaur-D1AR |
Launch site | Cape Canaveral LC-36A |
End of mission | |
Disposal | Decommissioned |
Last contact | October 8, 1992, 19:22 | UTC
Decay date | October 22, 1992[2] |
Orbital parameters | |
Reference system | Cytherocentric |
Semi-major axis | 33,405.8 kilometres (20,757.4 mi) |
Eccentricity | 0.842 |
Pericytherion altitude | 181.6 kilometers (112.8 mi) |
Apocytherion altitude | 66,630 kilometers (41,400 mi) |
Inclination | 105 degrees |
Period | 24 hours |
Epoch | 22 November 1979, 11:53:20 UTC[3] |
Venus orbiter | |
Orbital insertion | December 4, 1978 |
The Pioneer Venus Orbiter, also known as Pioneer Venus 1 or Pioneer 12, was a mission to Venus conducted by NASA as part of the Pioneer Venus project. Launched in May 1978 atop an Atlas-Centaur rocket, the spacecraft was inserted into an elliptical orbit around Venus on December 4, 1978. It returned data from Venus until October 1992.[2][4]
Launch and arrival at Venus
[edit]![](https://upload.wikimedia.org/wikipedia/commons/thumb/f/f4/Pioneer_Venus_1_orbit_attitude.gif/220px-Pioneer_Venus_1_orbit_attitude.gif)
The Pioneer Venus Orbiter was launched by an Atlas SLV-3D Centaur-D1AR rocket, which flew from Launch Complex 36A at the Cape Canaveral Air Force Station. The launch occurred at 13:13:00 (8:13 a.m. local time) on May 20, 1978, and deployed the Orbiter into heliocentric orbit for its coast to Venus. Venus orbit insertion occurred on December 4, 1978.
Spacecraft
[edit]![](https://upload.wikimedia.org/wikipedia/commons/thumb/6/6a/Pioneer_Venus_1_at_KSC.jpg/170px-Pioneer_Venus_1_at_KSC.jpg)
Manufactured by Hughes Aircraft Company, the Pioneer Venus Orbiter was based on the HS-507 bus.[5] The spacecraft was a flat cylinder, 2.5 meters (8.2 ft) in diameter and 1.2 meters (3.9 ft) long. All instruments and spacecraft subsystems were mounted on the forward end of the cylinder, except the magnetometer, which was at the end of a 4.7 meters (15 ft) boom. A solar array extended around the circumference of the cylinder. A 1.09 metres (3 ft 7 in) despun dish antenna provided S and X band communication with Earth. A Star-24 solid rocket motor was integrated into the spacecraft to provide the thrust to enter orbit around Venus.[5]
From Venus orbit insertion to July 1980, periapsis was held between 142 and 253 kilometres (88 and 157 mi) (at 17 degrees north latitude) to facilitate radar and ionospheric measurements. The spacecraft was in a 24-hour orbit with an apoapsis of 66,900 kilometers (41,600 mi). Thereafter, the periapsis was allowed to rise to a maximum of 2,290 kilometres (1,420 mi) and then fall, to conserve fuel.
In 1991, the Radar Mapper was reactivated to investigate previously inaccessible southern portions of the planet, in conjunction with the recently arrived Magellan spacecraft. In May 1992, Pioneer Venus began the final phase of its mission, in which the periapsis was held between 150 and 250 kilometres (93 and 155 mi), until the spacecraft's propellant was exhausted, after which the orbit decayed naturally. The spacecraft continued to return data until 8 October 1992, with the last signals being received at 19:22 UTC.[4] The Pioneer Venus Orbiter disintegrated upon entering the atmosphere of Venus on October 22, 1992.[2]
Instruments
[edit]![](https://upload.wikimedia.org/wikipedia/commons/thumb/d/dd/Venus_map_with_labels.jpg/190px-Venus_map_with_labels.jpg)
The Pioneer Venus Orbiter carried 17 experiments with a total mass of 45 kilograms (99 lb):[6]
![](https://upload.wikimedia.org/wikipedia/commons/thumb/6/64/Venus_clouds_seen_by_Pioneer_Venus_Orbiter.jpg/190px-Venus_clouds_seen_by_Pioneer_Venus_Orbiter.jpg)
- a cloud photo-polarimeter (OCPP) to measure the vertical distribution of the clouds, similar to Pioneer 10 and Pioneer 11 imaging photo-polarimeter (IPP)
- a surface radar mapper (ORAD) to determine topography and surface characteristics. Observations could only be conducted when the probe was closer than 4,700 kilometres (2,900 mi) over the planet. A 20-watt S-band signal (1.757 gigahertz) was sent to the surface that reflected it, with the probe analyzing the echo. Resolution at periapsis was 23 by 7 kilometres (14.3 mi × 4.3 mi).
- an infrared radiometer (OIR) to measure IR emissions from Venus' atmosphere
- an airglow ultraviolet spectrometer (OUVS) to measure scattered and emitted UV light
- a neutral mass spectrometer (ONMS) to determine the composition of the upper atmosphere
- a solar wind plasma analyzer (OPA) to measure properties of the solar wind
- a magnetometer (OMAG) to characterize the magnetic field at Venus
- an electric field detector (OEFD) to study the solar wind and its interactions
- an electron temperature probe (OETP) to study the thermal properties of the ionosphere
- an ion mass spectrometer (OIMS) to characterize the ionospheric ion population
- a charged particle retarding potential analyzer (ORPA) to study ionospheric particles
- two radio science experiments to determine the gravity field of Venus
- a radio occultation experiment to characterize the atmosphere
- an atmospheric drag experiment to study the upper atmosphere
- a radio science atmospheric and solar wind turbulence experiment
- a gamma ray burst (OGBD) detector to record gamma ray burst events
![](https://upload.wikimedia.org/wikipedia/commons/thumb/a/a7/Pioneer-Venus-Orbiter-orbit.png/190px-Pioneer-Venus-Orbiter-orbit.png)
![](https://upload.wikimedia.org/wikipedia/commons/thumb/1/1b/Atlas_Centaur_with_Pioneer_Venus_Orbiter.jpg/190px-Atlas_Centaur_with_Pioneer_Venus_Orbiter.jpg)
![](https://upload.wikimedia.org/wikipedia/commons/thumb/a/a2/Pioneer-Venus-Trajectories.png/190px-Pioneer-Venus-Trajectories.png)
Name | Complete designation | Type | Manufacturer | Responsible scientist | Mass | Electrical consumption |
---|---|---|---|---|---|---|
OCPP | Orbiter Cloud Photopolarimeter | Photo polarimeter | GISS | J. Hansen (later L. Travis) | 5 kg (11 lb) | 5.4 W |
ORAD | Orbiter Radar Mapper Instrument | Radar | MIT | G. Pettengill | 9 kg (20 lb) | 18 W |
OIR | Orbiter Infrared Radiometer | Infrared radiometer | JPL | F. Taylor | 5.9 kg (13 lb) | 5.2 W |
OUVS | Orbiter Ultraviolet Spectrometer | Ultraviolet spectrometer | LASP | A.I.F. Stewart | 3.1 kg (6.8 lb) | 1.7 W |
ONMS | Orbiter Neutral Mass Spectrometer | Neutral mass spectrometer | GSFC | H. Neimann | 3.8 kg (8.4 lb) | 12 W |
OPA | Orbiter Plasma Analyzer | Analzer plasma | ARC | J. Wolfe (later A. Barnes) | 3.9 kg (8.6 lb) | 5 W |
OMAG | Orbiter Magnetometer | Magnetometer | UCLA | C. Russell | 2 kg (4.4 lb) | 2.2 W |
OEFD | Orbiter Electric Field Detector | Measure the electric fields of Venus | TRW | F. Scarf | 0.8 kg (1.8 lb) | 0.7 W |
OETP | Orbiter Electron Temperature Probe | Electron temperature gauge | GSFC | L. Brace | 2.2 kg (4.9 lb) | 4.8 W |
OIMS | Orbiter Ion Mass Spectrometer | Ion mass spectrometer | GSFC | H. Taylor | 3 kg (6.6 lb) | 1.5 W |
ORPA | Orbiter Retarding Potential Analyzer | Ion charge meter | LPARL | W. Knudsen | 2.8 kg (6.2 lb) | 2.4 W |
OGBD | Orbiter Gamma-Ray Burst Detector | Gamma-ray burst detector | LASL | W. Evans | 2.8 kg (6.2 lb) | 1.3 W |
- | Venus (ORO) | Radio science | - | A. Kliore (JPL) | – | - |
Orbiter Dual-Frequency Experiments (OGPE) | - | T. Croft (SRI) | ||||
Atmospheric and Solar Wind Turbulence Experiment (OTUR) | - | T. Croft (JPL) | ||||
Orbiter Atmospheric Drag Experiment (OAD) | - | G. Keating (LRC) | ||||
Orbiter Internal Density Distribution Experiment (OIDD) | - | R. Phillips (JPL) | ||||
Orbiter Celestial Mechanics Experiment (OCM) | - | I. Shapiro (MIT) | ||||
LASP: Laboratory for Atmospheric and Space Physics (University of Boulder, Colorado); UCLA: University of California in Los Angeles; JPL: Jet Propulsion Laboratory; MIT: Massachusetts Institute of Technology; GSFC: Goddard Space Flight Center GISS: Goddard Institute for Space Studies; LRC: Langley Research Center; ARC: Ames Research Center; LASL: Los Alamos National Laboratory; SRI: Stanford Research Institute |
The spacecraft conducted radar altimetry observations allowing the first global topographic map of the Venusian surface to be constructed.
The instruments can also be classified by what they are meant to measure or analyze:[7]
- Composition and structure of the atmosphere
- Large Probe Mass Spectrometer (LNMS)
- Large Probe Gas Chromatograph (LGC)
- Bus Neutral Mass Spectrometer (BNMS)
- Orbiter Neutral Mass Spectrometer (ONMS)
- Orbiter Ultraviolet Spectrometer (OUVS)
- Large/Small Probe Atmosphere Structure (LAS/SAS)
- Atmospheric Propagation Experiments (OGPE)
- Orbiter Atmospheric Drag Experiment (OAD)
- Clouds
- Large/Small Probe Nephelometer (LN/SN)
- Large Probe Cloud Particle Size Spectrometer (LCPS)
- Orbiter Cloud Photopolarimenter (OCPP)
- Thermal balance
- Large Probe Solar Flux Radiometer (LSFR)
- Large Probe Infrared Radiometer (LIR)
- Small Probe Net Flux Radiometer (SNFR)
- Orbiter Infrared Radiometer (OIR)
- Dynamics
- Differential Long Baseline Interferometry (DLBI)
- Doppler Tracking of Probes (MWIN)
- Atmospheric Turbulence Experiments (MTUR/OTUR)
- Solar wind and ionosphere
- Bus Ion Mass Spectrometer (BIMS)
- Orbiter Ion Mass Spectrometer (OIMS)
- Orbiter Electron Temperature Probe (OETP)
- Orbiter Retarding Potential Analyzer (ORPA)
- Orbiter Magnetometer (OMAG)
- Orbiter Plasma Analyzer (OPA)
- Orbiter Electric Field Detector (OEFD)
- Orbiter Dual-Frequency Occultation Experiments (ORO)
- Surface and interior
- Orbiter Radar Mapper (ORAD)
- Orbiter Internal Density Distribution Experiments (OIDD)
- Orbiter Celestial Mechanics Experiments (OCM)
- High-energy astronomy
- Orbiter Gamma Burst Detector (OGBD)
Observations of Comets
[edit]From its orbit of Venus, the Pioneer Venus Orbiter was able to observe Halley's Comet when it was unobservable from Earth due to its proximity to the sun during February 1986. UV spectrometer observations monitored the loss of water from the comet's nucleus at perihelion on February 9.[8]
The extended mission allowed the spacecraft controllers to make several comet observations that were never part of the original mission objectives. The tilt of the spacecraft was altered during these comet observations so that the Ultraviolet Spectrometer (OUVS) could view the comets rather than Venus. Comets Encke (April 13–16, 1984), Giacobini-Zinner (September 8–15, 1985), Halley (December 27, 1985 - March 9, 1986), Wilson (March 13 - May 2, 1987), NTT (April 8, 1987), and McNaught (November 19–24, 1987) were all observed in this way.[7]
See also
[edit]- Pioneer Venus Multiprobe
- List of missions to Venus
- Timeline of artificial satellites and space probes
References
[edit]- ^ a b "Pioneer Venus Orbiter/Pioneer Venus 1/Pioneer 12". NASA's Solar System Exploration website. Retrieved December 1, 2022.
- ^ a b c McDowell, Jonathan. "Satellite Catalog". Jonathan's Space Page. Archived from the original on 2003-10-11.
- ^ "NASA - NSSDCA - Spacecraft - Trajectory Details". nssdc.gsfc.nasa.gov. Retrieved 2018-05-02.
- ^ a b "Pioneer Venus 1". Solar System Exploration. NASA. Archived from the original on 2006-10-04. Retrieved 2013-08-16.
- ^ a b Krebs, Gunter. "Pioneer 12 (Pioneer Venus Orbiter, PVO)". Gunter's Space Page. Archived from the original on 2005-01-12.
- ^ "Pioneer Venus Project Information". NASA Goddard Space Flight Center. Retrieved 2016-08-17.
- ^ a b "PVO Mission Document". NASA.
- ^ Russell, C.T.; Luhmann, J.G.; Scarf, F.L. (1985). "Pioneer Venus Observations during Comet Halley's Inferior Conjunction" (PDF). University of California, Los Angeles. Archived from the original (PDF) on 2009-02-27. Retrieved 2013-08-16.
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- Russell, C. T.; Elphic, R. C.; Slavin, J. A. (6 July 1979). "Initial Pioneer Venus Magnetic Field Results: Nightside Observations". Science. 205 (4401): 114–116. Bibcode:1979Sci...205..114R. doi:10.1126/science.205.4401.114. JSTOR 1748535. PMID 17778922. S2CID 24494352.
- Intriligator, D. S.; Collard, H. R.; Mihalov, J. D.; Whitten, R. C.; Wolfe, J. H. (6 July 1979). "Electron Observations and Ion Flows from the Pioneer Venus Orbiter Plasma Analyzer Experiment". Science. 205 (4401): 116–119. Bibcode:1979Sci...205..116I. doi:10.1126/science.205.4401.116. JSTOR 1748536. PMID 17778923. S2CID 42935022.
- Evans, W. D.; Glore, J. P.; Klebesadel, R. W.; Laros, J. G.; Tech, E. R.; Spalding, R. E. (6 July 1979). "Gamma-Ray Burst Observations by Pioneer Venus Orbiter". Science. 205 (4401): 119–121. Bibcode:1979Sci...205..119E. doi:10.1126/science.205.4401.119. JSTOR 1748537. PMID 17778924. S2CID 38916824.
- Donahue, T. M. (6 July 1979). "Pioneer Venus Results: An Overview". Science. 205 (4401): 41–44. Bibcode:1979Sci...205...41D. doi:10.1126/science.205.4401.41. JSTOR 1748508. PMID 17778895. S2CID 1600807.
- Colin, Lawrence (6 July 1979). "Encounter with Venus: An Update". Science. 205 (4401): 44–46. Bibcode:1979Sci...205...44C. doi:10.1126/science.205.4401.44. JSTOR 1748509. PMID 17778896. S2CID 26297893.
- Seiff, Alvin; Kirk, Donn B.; Young, Richard E.; Sommer, Simon C.; Blanchard, Robert C.; Findlay, John T.; Kelly, G. M. (6 July 1979). "Thermal Contrast in the Atmosphere of Venus: Initial Appraisal from Pioneer Venus Probe Data". Science. 205 (4401): 46–49. Bibcode:1979Sci...205...46S. doi:10.1126/science.205.4401.46. JSTOR 1748510. PMID 17778897. S2CID 24774892.
- Hoffman, J. H.; Hodges, R. R.; McElroy, M. B.; Donahue, T. M.; Kolpin, M. (6 July 1979). "Composition and Structure of the Venus Atmosphere: Results from Pioneer Venus". Science. 205 (4401): 49–52. Bibcode:1979Sci...205...49H. doi:10.1126/science.205.4401.49. JSTOR 1748511. PMID 17778898. S2CID 20713222.
- Oyama, V. I.; Carle, G. C.; Woeller, F.; Pollack, J. B. (6 July 1979). "Laboratory Corroboration of the Pioneer Venus Gas Chromatograph Analyses". Science. 205 (4401): 52–54. Bibcode:1979Sci...205...52O. doi:10.1126/science.205.4401.52. JSTOR 1748512. PMID 17778899. S2CID 40293580.
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