

Pioneer Venus Project Information

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.

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

a cloud photopolarimeter to measure the vertical distribution of the clouds

a surface radar mapper to determine topography and surface characteristics

an infrared radiometer to measure IR emissions from the Venus atmosphere

an airglow ultraviolet spectrometer to measure scattered and emitted UV light

a neutral mass spectrometer to determine the composition of the upper atmosphere

a solar wind plasma analyzer to measure properties of the solar wind

a magnetometer to characterize the magnetic field at Venus

an electric field detector to study the solar wind and its interactions

an electron temperature probe to study the thermal properties of the ionosphere

an ion mass spectrometer to characterize the ionospheric ion population

a charged particle retarding potential analyzer 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 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 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.

Detailed information on the orbiter, experiments, and data - NSSDCA Master Catalog

The Pioneer Venus Multiprobe consisted of a bus which carried one large and three small atmospheric probes. 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.

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

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 propogation 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.

More detailed information on the probes is available.

The Pioneer Venus bus also carried two experiments, a neutral mass spectromenter and an ion mass spectrometer to study the composition of the atmosphere. With no heat shield or parachute, the bus survived and made measurements only to about 110 km altitude before burning up. The bus was a 2.5 m diameter cylinder weighing 290 kg, and afforded the 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.

Detailed information on the probes, experiments, and data - NSSDCA Master Catalog



Other Pioneer Venus Information/Data at NSSDCA

Pioneer Venus Orbiter

Pioneer Venus Probe Bus

Pioneer Venus Large Probe

Pioneer Venus North Probe

Pioneer Venus Night Probe

Pioneer Venus Day Probe

COHOWeb - Browse and retrieve Pioneer Venus magnetic field data

SPDF anonymous FTP site

Related Information/Data at NSSDCA

Venus Page

Venus images in the NSSDCA Photo Gallery

Magellan Project



| NSSDCA Planetary page | Heliophysics page |

Author/Curator:

Dr. David R. Williams, dave.williams@nasa.gov

NSSDCA, Mail Code 690.1

NASA Goddard Space Flight Center

Greenbelt, MD 20771

+1-301-286-1258



NASA Official: Dr. David R. Williams, david.r.williams@nasa.gov

Last Updated: Monday, 10-Dec-2018 08:15:23 EST, EVB II