Pioneer Venus Orbiter

Last updated
Pioneer Venus Orbiter
Pioneer Venus orbiter.jpg
Artist's impression of Pioneer 12 in orbit above Venus
NamesPioneer Venus 1
Pioneer 12
Mission type Venus orbiter
Operator NASA  / Ames
COSPAR ID 1978-051A OOjs UI icon edit-ltr-progressive.svg
SATCAT no. 10911
Website science.nasa.gov
Mission durationTotal:
14 years, 4 months and 18 days
Science phase:
13 years, 10 months and 4 days
Spacecraft properties
Bus HS-507
Manufacturer Hughes
Launch mass582 kg (1,283 lb) [1]
Dry mass517 kg (1,140 lb)
Dimensions2.5 × 2.5 × 1.2 m (8.2 × 8.2 × 3.9 ft)
Power312 watts
Start of mission
Launch dateMay 20, 1978, 13:13:00 (1978-05-20UTC13:13Z) UTC [1]
Rocket Atlas SLV-3D Centaur-D1AR (AC-50)
Launch site Cape Canaveral LC-36A
End of mission
DisposalDecommissioned
Last contactOctober 8, 1992, 19:22 (1992-10-08UTC19:23Z) UTC
Decay dateOctober 22, 1992 [2]
Orbital parameters
Reference system Cytherocentric
Semi-major axis 33,405.8 km (20,757.4 mi)
Eccentricity 0.842
Pericytherion altitude 181.6 km (112.8 mi)
Apocytherion altitude 66,630 km (41,400 mi)
Inclination 105 degrees
Period 24 hours
Epoch 22 November 1979, 11:53:20 UTC [3]
Venus orbiter
Orbital insertionDecember 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]

Contents

Launch and arrival at Venus

Orbit attitude of Pioneer Venus 1 between 1978-1980 and 1992 Pioneer Venus 1 orbit attitude.gif
Orbit attitude of Pioneer Venus 1 between 1978–1980 and 1992

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

Pioneer Venus 1 at KSC. Pioneer Venus 1 at KSC.jpg
Pioneer Venus 1 at KSC.

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

A map of Venus produced from Pioneer data Venus map with labels.jpg
A map of Venus produced from Pioneer data

The Pioneer Venus Orbiter carried 17 experiments with a total mass of 45 kilograms (99 lb): [6]

An image of Venus in ultraviolet light by the Pioneer Venus Orbiter Venus clouds seen by Pioneer Venus Orbiter.jpg
An image of Venus in ultraviolet light by the Pioneer Venus Orbiter
Orbit of the spacecraft Pioneer Venus Orbiter. Pioneer-Venus-Orbiter-orbit.png
Orbit of the spacecraft Pioneer Venus Orbiter.
Launch of Pioneer Venus Orbiter with Atlas-Centaur rocket. Atlas Centaur with Pioneer Venus Orbiter.jpg
Launch of Pioneer Venus Orbiter with Atlas-Centaur rocket.
Trajectory of Pioneer Venus Orbiter. Pioneer-Venus-Trajectories.png
Trajectory of Pioneer Venus Orbiter.
Instrument details
NameComplete designationTypeManufacturerResponsible scientistMassElectrical consumption
OCPPOrbiter Cloud PhotopolarimeterPhoto polarimeterGISSJ. Hansen (later L. Travis)5 kg (11 lb)5.4 W
ORADOrbiter Radar Mapper InstrumentRadarMITG. Pettengill9 kg (20 lb)18 W
OIROrbiter Infrared RadiometerInfrared radiometerJPLF. Taylor5.9 kg (13 lb)5.2 W
OUVSOrbiter Ultraviolet SpectrometerUltraviolet spectrometerLASPA.I.F. Stewart3.1 kg (6.8 lb)1.7 W
ONMSOrbiter Neutral Mass SpectrometerNeutral mass spectrometerGSFCH. Neimann3.8 kg (8.4 lb)12 W
OPAOrbiter Plasma AnalyzerAnalzer plasmaARCJ. Wolfe (later A. Barnes)3.9 kg (8.6 lb)5 W
OMAGOrbiter MagnetometerMagnetometerUCLAC. Russell2 kg (4.4 lb)2.2 W
OEFDOrbiter Electric Field DetectorMeasure the electric fields of VenusTRWF. Scarf0.8 kg (1.8 lb)0.7 W
OETPOrbiter Electron Temperature ProbeElectron temperature gaugeGSFCL. Brace2.2 kg (4.9 lb)4.8 W
OIMSOrbiter Ion Mass SpectrometerIon mass spectrometerGSFCH. Taylor3 kg (6.6 lb)1.5 W
ORPAOrbiter Retarding Potential AnalyzerIon charge meterLPARLW. Knudsen2.8 kg (6.2 lb)2.4 W
OGBDOrbiter Gamma-Ray Burst DetectorGamma-ray burst detectorLASLW. Evans2.8 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]

Observations of Comets

Comet Halley by Pioneer Venus Orbiter Comet Halley by Pioneer 12 118532main AC86-0107-5.jpg
Comet Halley by Pioneer Venus Orbiter
Comet Wilson by Pioneer Venus Orbiter Comet Wilson by Pioneer 12 118534main AC87-0264-1.jpg
Comet Wilson by Pioneer Venus Orbiter

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

Related Research Articles

<span class="mw-page-title-main">Hydroxy group</span> Chemical group (–OH)

In chemistry, a hydroxy or hydroxyl group is a functional group with the chemical formula −OH and composed of one oxygen atom covalently bonded to one hydrogen atom. In organic chemistry, alcohols and carboxylic acids contain one or more hydroxy groups. Both the negatively charged anion HO, called hydroxide, and the neutral radical HO·, known as the hydroxyl radical, consist of an unbonded hydroxy group.

<span class="mw-page-title-main">Venus</span> Second planet from the Sun

Venus is the second planet from the Sun. It is a terrestrial planet and is the closest in mass and size to its orbital neighbour Earth. Venus has by far the densest atmosphere of the terrestrial planets, composed mostly of carbon dioxide with a thick, global sulfuric acid cloud cover. At the surface it has a mean temperature of 737 K and a pressure 92 times that of Earth's at sea level. These extreme conditions compress carbon dioxide into a supercritical state at Venus's surface.

<span class="mw-page-title-main">Mariner 2</span> First successful mission to Venus (1962–1963)

Mariner 2, an American space probe to Venus, was the first robotic space probe to report successfully from a planetary encounter. The first successful spacecraft in the NASA Mariner program, it was a simplified version of the Block I spacecraft of the Ranger program and an exact copy of Mariner 1. The missions of the Mariner 1 and 2 spacecraft are sometimes known as the Mariner R missions. Original plans called for the probes to be launched on the Atlas-Centaur, but serious developmental problems with that vehicle forced a switch to the much smaller Agena B second stage. As such, the design of the Mariner R vehicles was greatly simplified. Far less instrumentation was carried than on the Soviet Venera probes of this period—for example, forgoing a TV camera—as the Atlas-Agena B had only half as much lift capacity as the Soviet 8K78 booster. The Mariner 2 spacecraft was launched from Cape Canaveral on August 27, 1962, and passed as close as 34,773 kilometers (21,607 mi) to Venus on December 14, 1962.

<i>Mariner 10</i> First spacecraft to visit Mercury (1973–1975)

Mariner 10 was an American robotic space probe launched by NASA on 3 November 1973, to fly by the planets Mercury and Venus. It was the first spacecraft to perform flybys of multiple planets.

<i>Cassini–Huygens</i> NASA/ESA mission sent to study Saturn and its moons (1997–2017)

Cassini–Huygens, commonly called Cassini, was a space-research mission by NASA, the European Space Agency (ESA), and the Italian Space Agency (ASI) to send a space probe to study the planet Saturn and its system, including its rings and natural satellites. The Flagship-class robotic spacecraft comprised both NASA's Cassini space probe and ESA's Huygens lander, which landed on Saturn's largest moon, Titan. Cassini was the fourth space probe to visit Saturn and the first to enter its orbit, where it stayed from 2004 to 2017. The two craft took their names from the astronomers Giovanni Cassini and Christiaan Huygens.

<span class="mw-page-title-main">Pioneer Venus project</span> Two spacecraft send to Venus in 1978

The Pioneer Venus project was part of the Pioneer program consisting of two spacecraft, the Pioneer Venus Orbiter and the Pioneer Venus Multiprobe, launched to Venus in 1978. The program was managed by NASA's Ames Research Center.

<i>MESSENGER</i> NASA mission to Mercury

MESSENGER was a NASA robotic space probe that orbited the planet Mercury between 2011 and 2015, studying Mercury's chemical composition, geology, and magnetic field. The name is a backronym for Mercury Surface, Space Environment, Geochemistry, and Ranging, and a reference to the messenger god Mercury from Roman mythology.

<span class="mw-page-title-main">Pioneer Venus Multiprobe</span> NASA atmospheric mission to Venus (1978)

The Pioneer Venus Multiprobe, also known as Pioneer Venus 2 or Pioneer 13, was a spacecraft launched in 1978 to explore Venus as part of NASA's Pioneer program. This part of the mission included a spacecraft bus which was launched from Earth carrying one large and three smaller probes, which after separating penetrated the Venusian atmosphere at a different location, returning data as they descended into the planet's thick atmosphere. The entry occurred on December 9, 1978.

<i>Venus Express</i> European orbiter mission to Venus (2005–2015)

Venus Express (VEX) was the first Venus exploration mission of the European Space Agency (ESA). Launched in November 2005, it arrived at Venus in April 2006 and began continuously sending back science data from its polar orbit around Venus. Equipped with seven scientific instruments, the main objective of the mission was the long term observation of the Venusian atmosphere. The observation over such long periods of time had never been done in previous missions to Venus, and was key to a better understanding of the atmospheric dynamics. ESA concluded the mission in December 2014.

<span class="mw-page-title-main">Io (moon)</span> Innermost of the four Galilean moons of Jupiter

Io, or Jupiter I, is the innermost and second-smallest of the four Galilean moons of the planet Jupiter. Slightly larger than Earth's moon, Io is the fourth-largest moon in the Solar System, has the highest density of any moon, the strongest surface gravity of any moon, and the lowest amount of water by atomic ratio of any known astronomical object in the Solar System. It was discovered in 1610 by Galileo Galilei and was named after the mythological character Io, a priestess of Hera who became one of Zeus's lovers.

<span class="mw-page-title-main">Venera 4</span> 1967 Soviet Venus probe

Venera 4, also designated 4V-1 No.310, was a probe in the Soviet Venera program for the exploration of Venus. The probe comprised a lander, designed to enter the Venusian atmosphere and parachute to the surface, and a carrier/flyby spacecraft, which carried the lander to Venus and served as a communications relay for it.

<span class="mw-page-title-main">Observations and explorations of Venus</span>

Observations of the planet Venus include those in antiquity, telescopic observations, and from visiting spacecraft. Spacecraft have performed various flybys, orbits, and landings on Venus, including balloon probes that floated in the atmosphere of Venus. Study of the planet is aided by its relatively close proximity to the Earth, compared to other planets, but the surface of Venus is obscured by an atmosphere opaque to visible light.

<span class="mw-page-title-main">Max Planck Institute for Solar System Research</span>

The Max Planck Institute for Solar System Research is a research institute in astronomy and astrophysics located in Göttingen, Germany, where it relocated in February 2014 from the nearby village of Lindau. The exploration of the Solar System is the central theme for research done at this institute.

<span class="mw-page-title-main">Atmosphere of Venus</span> Gas layer surrounding Venus

The atmosphere of Venus is the very dense layer of gases surrounding the planet Venus. Venus's atmosphere is composed of 96.5% carbon dioxide and 3.5% nitrogen, with other chemical compounds present only in trace amounts. It is much denser and hotter than that of Earth; the temperature at the surface is 740 K, and the pressure is 93 bar (1,350 psi), roughly the pressure found 900 m (3,000 ft) under water on Earth. The atmosphere of Venus supports decks of opaque clouds of sulfuric acid that cover the entire planet, preventing optical Earth-based and orbital observation of the surface. Information about surface topography has been obtained exclusively by radar imaging.

<span class="mw-page-title-main">Exploration of Jupiter</span> Overview of the exploration of Jupiter the planet and its moons

The exploration of Jupiter has been conducted via close observations by automated spacecraft. It began with the arrival of Pioneer 10 into the Jovian system in 1973, and, as of 2024, has continued with eight further spacecraft missions in the vicinity of Jupiter and two more en route. All but one of these missions were undertaken by the National Aeronautics and Space Administration (NASA), and all but four were flybys taking detailed observations without landing or entering orbit. These probes make Jupiter the most visited of the Solar System's outer planets as all missions to the outer Solar System have used Jupiter flybys. On 5 July 2016, spacecraft Juno arrived and entered the planet's orbit—the second craft ever to do so. Sending a craft to Jupiter is difficult, mostly due to large fuel requirements and the effects of the planet's harsh radiation environment.

<span class="mw-page-title-main">Atmosphere of Titan</span>

The atmosphere of Titan is the dense layer of gases surrounding Titan, the largest moon of Saturn. Titan is the only natural satellite of a planet in the Solar System with an atmosphere that is denser than the atmosphere of Earth and is one of two moons with an atmosphere significant enough to drive weather. Titan's lower atmosphere is primarily composed of nitrogen (94.2%), methane (5.65%), and hydrogen (0.099%). There are trace amounts of other hydrocarbons, such as ethane, diacetylene, methylacetylene, acetylene, propane, PAHs and of other gases, such as cyanoacetylene, hydrogen cyanide, carbon dioxide, carbon monoxide, cyanogen, acetonitrile, argon and helium. The isotopic study of nitrogen isotopes ratio also suggests acetonitrile may be present in quantities exceeding hydrogen cyanide and cyanoacetylene. The surface pressure is about 50% higher than on Earth at 1.5 bars which is near the triple point of methane and allows there to be gaseous methane in the atmosphere and liquid methane on the surface. The orange color as seen from space is produced by other more complex chemicals in small quantities, possibly tholins, tar-like organic precipitates.

<span class="mw-page-title-main">MAVEN</span> NASA Mars orbiter (2013–Present)

MAVEN is a NASA spacecraft orbiting Mars to study the loss of that planet's atmospheric gases to space, providing insight into the history of the planet's climate and water. The name is an acronym for "Mars Atmosphere and Volatile Evolution" while the word maven also denotes "a person who has special knowledge or experience; an expert". MAVEN was launched on an Atlas V rocket from Cape Canaveral Air Force Station, Florida, on 18 November 2013 UTC and went into orbit around Mars on 22 September 2014 UTC. The mission is the first by NASA to study the Mars atmosphere. The probe is analyzing the planet's upper atmosphere and ionosphere to examine how and at what rate the solar wind is stripping away volatile compounds.

<span class="mw-page-title-main">Exploration of Io</span> Overview of the exploration of Io, Jupiters innermost Galilean and third-largest moon

The exploration of Io, Jupiter's innermost Galilean and third-largest moon, began with its discovery in 1610 and continues today with Earth-based observations and visits by spacecraft to the Jupiter system. Italian astronomer Galileo Galilei was the first to record an observation of Io on January 8, 1610, though Simon Marius may have also observed Io at around the same time. During the 17th century, observations of Io and the other Galilean satellites helped with the measurement of longitude by map makers and surveyors, with validation of Kepler's Third Law of planetary motion, and with measurement of the speed of light. Based on ephemerides produced by astronomer Giovanni Cassini and others, Pierre-Simon Laplace created a mathematical theory to explain the resonant orbits of three of Jupiter's moons, Io, Europa, and Ganymede. This resonance was later found to have a profound effect on the geologies of these moons. Improved telescope technology in the late 19th and 20th centuries allowed astronomers to resolve large-scale surface features on Io as well as to estimate its diameter and mass.

<span class="mw-page-title-main">Earth analog</span> Planet with environment similar to Earths

An Earth analog, also called an Earth analogue, Earth twin, or second Earth, is a planet or moon with environmental conditions similar to those found on Earth. The term Earth-like planet is also used, but this term may refer to any terrestrial planet.

Sushil K. Atreya is a planetary scientist, educator, and researcher. Atreya is a professor of Climate and Space Sciences and Engineering at the University of Michigan, Ann Arbor.

References

  1. 1 2 "Pioneer Venus Orbiter/Pioneer Venus 1/Pioneer 12". NASA's Solar System Exploration website. Retrieved December 1, 2022.
  2. 1 2 3 McDowell, Jonathan. "Satellite Catalog". Jonathan's Space Page. Archived from the original on 2003-10-11.
  3. "NASA - NSSDCA - Spacecraft - Trajectory Details". nssdc.gsfc.nasa.gov. Retrieved 2018-05-02.
  4. 1 2 "Pioneer Venus 1". Solar System Exploration. NASA. Archived from the original on 2006-10-04. Retrieved 2013-08-16.
  5. 1 2 Krebs, Gunter. "Pioneer 12 (Pioneer Venus Orbiter, PVO)". Gunter's Space Page. Archived from the original on 2005-01-12.
  6. "Pioneer Venus Project Information". NASA Goddard Space Flight Center. Retrieved 2016-08-17.
  7. 1 2 "PVO Mission Document". NASA.
  8. 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.

Bibliography