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Pioneer Venus project

By Wikipedia,
the free encyclopedia,

http://en.wikipedia.org/wiki/Pioneer_Venus

Pioneer Venus Orbiter

Pioneer Venus Orbiter
Organization Ames Research Center - NASA
Mission type Orbiter
Satellite of Venus
Orbital insertion date December 4, 1978
Launch date 20 May 1978
Launch vehicle Atlas-Centaur
Mission duration 20 May 1978 to August, 1992
Orbital decay August, 1992
COSPAR ID 1978-051A
Home page National Space Science Data Center (NASA)
Mass 517 kg
Power 312 W
Orbital elements
Eccentricity .842
Inclination 105°
Orbital period 24 h
Apoapsis 1.03 RV
Periapsis 12.01 RV

The Pioneer mission to Venus consisted of two components, launched separately. Pioneer Venus 1 or Pioneer Venus Orbiter was launched in 1978 and studied the planet for more than a decade after orbital insertion in 1978. Pioneer Venus 2 or Pioneer Venus Multiprobe sent four small probes into the Venusian atmosphere. This was managed by NASA Ames Research Center as part of the Pioneer series of spacecraft that included Pioneer 10 and Pioneer 11.

Pioneer Venus Orbiter

The Pioneer Venus Orbiter was inserted into an elliptical orbit around Venus on December 4, 1978. The Orbiter was a flat cylinder 2.5 m in diameter and 1.2 m high. 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 m boom. A solar array extended around the circumference of the cylinder. A 1.09 m despun dish antenna provided S and X band communication with Earth. It was manufactured by Hughes Aircraft Company.

The Pioneer Venus Orbiter carried 17 experiments (with a total mass of 45 kg):

  • 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 4700 km 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 x 7 km.
  • 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

From Venus orbit insertion to July 1980, periapsis was held between 142 and 253 km (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 km. Thereafter, the periapsis was allowed to rise (to 2290 km at maximum) 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 probe. In May 1992 Pioneer Venus began the final phase of its mission, in which the periapsis was held between 150 and 250 km, until the fuel ran out and atmospheric entry destroyed the spacecraft the following August.

Pioneer Venus Multiprobe


Pioneer Venus Multiprobe
Pioneer Venus Multiprobe

Pioneer Venus Large Probe
Pioneer Venus Large Probe
  • Launch Date: 8 August 1978
  • Launch Vehicle: Atlas-Centaur
  • Mass: 290 kg (bus), 315 kg (large probe), 90 kg (each small probe)
  • Power System: Solar Array of 241 W (bus), Batteries (probes)

The Pioneer Venus Multiprobe consisted of a bus which carried one large and three small atmospheric probes. None of these atmospheric probes had photographic imaging capabilities and were not designed for soil analysis. They weren't even designed for a soft landing; the large probe had a parachute that was designed to cut loose at a certain altitude, and the small probes had no parachute at all. Survival to the surface was considered a bonus. All the entry probes survived the density of the Venusian atmosphere at least until impact, but only one probe survived for a significant period after impact.

The large probe was released on November 16, 1978 and the three small probes on November 20. All four probes entered the Venus atmosphere on December 9, followed by the bus.

Pioneer Venus Probes and Bus: Atmospheric Entry and Impacts (all times in UT)
Large Probe North Probe Day Probe Night Probe Bus
Entry Time (200 km) 18:45:32 18:49:40 18:52:18 18:56:13 20:21:52
Impact Time 19:39:53 19:42:40 19:47:59 19:52:05 (signal lost at 110 km altitude)
Loss of Signal 19:39:53 19:42:40 20:55:34 19:52:07 20:22:55
Impact Latitude 4.4 N 59.3 N 31.3 S 28.7 S (37.9 S)
Impact Longitude 304.0 4.8 317.0 56.7 (290.9)
Solar Zenith Angle 65.7 108.0 79.9 150.7 60.7
Local Venus Time 7:38 3:35 6:46 0:07 8:30

Bus

The Pioneer Venus bus portion of the spacecraft was targeted to enter the Venusian atmosphere at a shallow entry angle and transmit data until destruction by the heat of atmospheric friction. The objective was to study the structure and composition of the atmosphere down to the surface, the nature and composition of the clouds, the radiation field and energy exchange in the lower atmosphere, and local information on the atmospheric circulation pattern.

The bus was a 2.5 m diameter cylinder weighing 290 kg, and afforded us our only direct view of the upper Venus atmosphere, as the probes did not begin making direct measurements until they had decelerated lower in the atmosphere.

With no heat shield or parachute, the bus made upper atmospheric measurements with two instruments, an Ion Mass Spectrometer (BIMS) and a Neutral Mass Spectrometer (BNMS), up to an altitude of about 165 km before disintegrating on December 9, 1978.

Large probe


Large probe (1-radio-transparent window, 2-tail protection, 3-antenna, 4-hermetic container, 5-sensors, 6-frontal protection)
Large probe (1-radio-transparent window, 2-tail protection, 3-antenna, 4-hermetic container, 5-sensors, 6-frontal protection)

The Pioneer Venus Large probe was equipped with 7 science experiments, contained within a sealed spherical pressure vessel. The science experiments were:

  • a neutral mass spectrometer to measure the atmospheric composition
  • a gas chromatograph to measure the atmospheric composition
  • a solar flux radiometer to measure solar flux penetration in the atmosphere
  • an infrared radiometer to measure distribution of infrared radiation
  • a cloud particle size spectrometer to measure particle size and shape
  • a nephelometer to search for cloud particles
  • temperature, pressure, and acceleration sensors

This pressure vessel was encased in a nose cone and aft protective cover. After deceleration from initial atmospheric entry at about 11.5 km/s near the equator on the Venus night side, a parachute was deployed at 47 km altitude. The large probe was about 1.5 m in diameter and the pressure vessel itself was 73.2 cm in diameter.

Small probes


Small probe. (1-antenna, 2-temperature sensor, 3-frontal protection, 4-hermetic container, 5-nephelometer, 6-radiometer)
Small probe. (1-antenna, 2-temperature sensor, 3-frontal protection, 4-hermetic container, 5-nephelometer, 6-radiometer)

The three small probes were identical to each other, 0.8 m in diameter. These probes also consisted of spherical pressure vessels surrounded by an aeroshell, but unlike the large probe, they had no parachutes and the aeroshells did not separate from the probe.

Each small probe carried a nephelometer and temperature, pressure, and acceleration sensors, as well as a net flux radiometer experiment to map the distribution of sources and sinks of radiative energy in the atmosphere. The radio signals from all four probes were also used to characterize the winds, turbulence, and propagation in the atmosphere.

The small probes were each targeted at different parts of the planet and were named accordingly.

  • The North probe entered the atmosphere at about 60 degrees north latitude on the day side.
  • The Night probe entered on the night side.
  • The Day probe entered well into the day side, and was the only one of the four probes which continued to send radio signals back after impact, for over an hour.

Halley's Comet in 1986

Pioneer Venus Orbiter orbiting Venus had a front row seat when Halley's Comet was more or less hidden behind the Sun during February 1986. Its UV-spectrometer observed the water loss when Halley's Comet was at perihelion February 9th.

See also

  1. ^ "Pioneer Venus Observations during Comet Halley's Inferior Conjunction". University of California, Los Angeles. http://www-ssc.igpp.ucla.edu/personnel/russell/papers/pioneerVenus_conjunct.pdf. Retrieved on 2009-02-10. 

External links




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Published - July 2009














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