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— CH. 1 · INTRODUCTION —

Pioneer 11

~7 min read · Ch. 1 of 7
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  • Pioneer 11 lifted off from Space Launch Complex 36A at Cape Canaveral, Florida, on the 6th of April 1973, at 02:11:00 UTC, riding an Atlas-Centaur rocket into the predawn sky. Its destination was the outer Solar System, a region no spacecraft had reached before. At the time of launch, humans had never seen Saturn from close range. No probe had threaded the asteroid belt and survived. The very first question Pioneer 11 had to answer was whether the journey through that belt was even survivable. Beyond that waited Jupiter, Saturn, and ultimately the void between the stars. This is the story of a probe that weighed 259 kilograms and carried twelve scientific instruments into territory no machine had visited before.

  • NASA approved the Pioneer 11 mission in February 1969, alongside its twin, Pioneer 10. Together they were the first probes designed specifically for the outer Solar System. TRW built the spacecraft, and NASA Ames Research Center managed the program. The hexagonal bus at Pioneer 11's core measured 36 centimeters deep, with six panels each 76 centimeters wide. Everything the probe needed to survive had to fit within that frame or be attached to it.

    Power was one of the central engineering challenges. Pioneer 11 carried four SNAP-19 radioisotope thermoelectric generators, mounted on two trusses each 3 meters long and separated by 120 degrees. At launch they produced 155 watts combined. By the time the probe reached Jupiter, that had already decayed to 140 watts. The spacecraft needed 100 watts just to run all its systems, leaving a thin margin for the instruments.

    Communication with Earth depended on a pair of transceivers, each transmitting at 8 watts across the S-band. The uplink from Earth ran at 2110 MHz; the downlink home used 2292 MHz. Because the distances involved were so vast, the Deep Space Network tracked the signal. Before transmitting, the probe ran data through a convolutional encoder so that errors could be corrected on the ground. The onboard computer was extremely limited, holding only five commands in memory at a time from a total possible set of 222 entries. Mission operators had to plan commands far in advance, and a data storage unit with a capacity of just 6,144 bytes held what the instruments gathered before transmission.

    Orientation in deep space was maintained with six 4.5-newton hydrazine thrusters, grouped in three pairs. One pair kept the probe spinning at 4.8 revolutions per minute. The spacecraft tracked Earth with conical scanning maneuvers and referenced the star Canopus with a dedicated sensor. Its backup, Pioneer H, now sits in the Milestones of Flight exhibit at the National Air and Space Museum in Washington, D.C.

  • One of the founding questions of the Pioneer program was whether any spacecraft could pass through the asteroid belt intact. Scientists in the 1960s genuinely did not know how dense the belt was in terms of debris. Pioneer 11 was the second probe to attempt the crossing, following Pioneer 10, and the fact that both emerged undamaged told mission planners something important: the outer Solar System was reachable.

    Pioneer 11 carried twelve scientific instruments to study what it encountered. The Meteoroid Detectors consisted of twelve panels of pressurized cells mounted on the back of the main dish antenna, recording direct impacts. The Asteroid and Meteoroid Detector looked outward through four non-imaging telescopes, tracking particles ranging from nearby dust to distant large asteroids. Together they gave scientists their first in-situ census of debris between Mars and Jupiter. That data mattered not just for Pioneer itself, but as a planning resource for every subsequent outer-planet mission.

  • Pioneer 11 flew past Jupiter in November and December 1974. At its closest approach on December 2, it passed 42,828 kilometers above the cloud tops. No probe had ever been this close to the largest planet in the Solar System, and what it returned was extraordinary. Detailed images of the Great Red Spot came back for the first time from spacecraft range. The probe transmitted the first images of Jupiter's immense polar regions. Its instruments also pinned down the mass of Callisto, Jupiter's outermost large moon, by measuring how that moon's gravity tugged at the passing probe.

    The encounter was not only scientific. It was also a navigation maneuver. Mission planners used Jupiter's enormous gravitational pull to bend Pioneer 11's trajectory and accelerate it toward Saturn, a technique called a gravity assist. In May 1974, before the Jupiter flyby, the probe had been retargeted onto a north-south path that would enable a Saturn encounter in 1979. That retargeting burn used 17 pounds of propellant, lasted 42 minutes and 36 seconds, and boosted Pioneer 11's speed by 230 kilometers per hour. Two mid-course corrections, on April 11 and November 7 of 1974, refined the path further. On the 16th of April 1975, after Jupiter was behind it, the micrometeoroid detector was switched off to conserve power.

  • Pioneer 11 reached Saturn on the 1st of September 1979, passing 21,000 kilometers from the planet's cloud tops. By that point, Voyager 1 and Voyager 2 had already swept past Jupiter and were racing toward Saturn on their own trajectories. That timing created a specific problem. Voyager 2's path to Uranus and Neptune required it to cross the Saturn ring plane at a particular position. Mission planners made a deliberate choice: send Pioneer 11 through that exact position first, so that if it was destroyed by ring debris, Voyager 2 could be redirected to a safer path before reaching Saturn.

    The rings themselves looked different up close than they did from Earth. Seen from the ground, Saturn's rings appear bright while the gaps between them look dark. Pioneer's pictures reversed that relationship: the rings appeared dark, and the gaps glowed bright. Pioneer also measured the atmosphere of Saturn's largest moon, Titan, and determined that it was too cold to support life as scientists understood it. The probe also charted Saturn's magnetosphere and mapped its magnetic field.

  • On the 25th of February 1990, Pioneer 11 became the fourth human-made object to cross beyond the orbit of the outermost planets. By 1995, the RTGs had decayed to the point that Pioneer 11 could no longer power any of its detectors. NASA Ames Research Center issued a press release on September 29 of that year, quoting NASA Administrator Daniel Goldin describing the probe as "the little spacecraft that could."

    Routine contact ended the following day, the 30th of September 1995. Scientists continued to listen for the spacecraft about once or twice a month, until the 24th of November 1995, when a final few minutes of good engineering data came through. Then Earth's own motion carried the planet out of view of Pioneer 11's antenna, and contact was lost for good.

    As of the 24th of June 2024, Pioneer 11 was estimated to be 113.121 AU from Earth, traveling at 11.155 kilometers per second relative to the Sun and moving outward at roughly 2.35 AU per year. The spacecraft is heading toward the constellation Scutum, near the open cluster Messier 26. Both Voyager probes, launched in 1977, have since overtaken Pioneer 11. Voyager 1 is now the most distant human-made object ever built.

    Pioneer 11 did leave behind one enduring puzzle. Analysis of radio tracking data from both Pioneer 10 and 11, at distances between 20 and 70 AU, revealed a small but consistent anomalous drift in their Doppler signals. Interpreted as an acceleration of (8.74 plus or minus 1.33) times ten to the negative-tenth meters per second squared, directed toward the Sun, this became known as the Pioneer anomaly. It occupied researchers for years. Extended analysis by Slava Turyshev and colleagues eventually traced the source to asymmetric thermal radiation and the resulting thermal recoil force acting on the face of the probes away from the Sun. In about 928,000 years, Pioneer 11 will pass within 0.25 parsecs of the K-dwarf star TYC 992-192-1.

  • Bolted to Pioneer 11's frame were two gold-anodized aluminum plaques, identical to the ones on Pioneer 10. They were designed as a message in case either spacecraft was ever intercepted by intelligent beings from another planetary system. The plaques show nude figures of a human male and female alongside symbols intended to communicate the probe's origin. The decision to include them reflected a particular moment in human thinking about space, when the reach of these probes made the prospect of them traveling indefinitely through the galaxy a real, not hypothetical, event.

    Back on Earth, Pioneer 11's achievements were recognized on one of ten United States Postage Service stamps issued in 1991, commemorating uncrewed spacecraft that had explored each of the then-nine planets and the Moon. Pioneer 11 was paired with Jupiter on that stamp. Pluto's stamp bore the words "Not yet explored." A full backup spacecraft, Pioneer H, was never launched; it now stands in the Milestones of Flight gallery in Washington, D.C., as a tangible record of what the mission required to build.

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Common questions

When was Pioneer 11 launched and by what rocket?

Pioneer 11 launched on the 6th of April 1973, at 02:11:00 UTC, from Space Launch Complex 36A at Cape Canaveral, Florida, aboard an Atlas-Centaur rocket with a Star-37E propulsion module.

What was Pioneer 11 the first spacecraft to do?

Pioneer 11 was the first spacecraft to encounter Saturn, passing 21,000 kilometers from its cloud tops on the 1st of September 1979. It was also the second probe to fly through the asteroid belt and the second to fly by Jupiter.

Why did Pioneer 11 fly through Saturn's ring plane at that specific position?

Mission planners directed Pioneer 11 through the exact ring-plane position that Voyager 2 would later need to cross on its way to Uranus and Neptune. If Pioneer 11 had been destroyed by ring debris, Voyager 2 could have been redirected to a safer path.

When did NASA lose contact with Pioneer 11?

Routine contact with Pioneer 11 ended on the 30th of September 1995. The last good engineering data was received on the 24th of November 1995, after which Earth moved out of view of the spacecraft's antenna.

What is the Pioneer anomaly and how was it explained?

The Pioneer anomaly was a small but unexplained acceleration of approximately 8.74 times ten to the negative-tenth meters per second squared directed toward the Sun, detected in radio tracking data from both Pioneer 10 and 11. Slava Turyshev and colleagues determined the cause was asymmetric thermal radiation and thermal recoil force acting on the face of the probes away from the Sun.

How far from Earth is Pioneer 11 now and where is it heading?

As of the 24th of June 2024, Pioneer 11 was estimated to be 113.121 AU from Earth, traveling at 11.155 kilometers per second relative to the Sun. It is heading toward the constellation Scutum and in approximately 928,000 years will pass within 0.25 parsecs of the star TYC 992-192-1.

All sources

35 references cited across the entry

  1. 1encyclopediaPioneer 10-11M. Wade
  2. 2journalFuture Stellar Flybys of the Voyager and Pioneer spacecraftC. A. L. Bailer-Jones et al. — 3 April 2019
  3. 3encyclopediaHardware, Leaving the Solar System: Where are they now?2001
  4. 5magazineFarewell to a PioneerSociety for Science — 14 October 1995
  5. 7newsSpace Launches are FeaturedS. Kronish — 27 October 1991
  6. 8webPioneer 11 - NASA ScienceNASA — December 21, 2017
  7. 10webPioneer 11 to End Operations after Epic CareerD. Savage et al. — NASA / Ames — 28 September 1995
  8. 11webPioneer 11: Magnetic FieldsE. J. Smith — NASA
  9. 14webPioneer 11: Cosmic-Ray SpectraF. B. MacDonald — NASA
  10. 15webPioneer 11: Geiger Tube Telescope (GTT)J. A. Van Allen — NASA
  11. 16webPioneer 11: Jovian Trapped RadiationR. W. Fillius — NASA
  12. 17webPioneer 11: Meteoroid DetectorsW. H. Kinard — NASA
  13. 18webPioneer 11: Asteroid/Meteoroid AstronomyR. K. Soberman — NASA
  14. 19webPioneer 11: Ultraviolet PhotometryD. L. Judge — NASA
  15. 21webPioneer 11: Infrared RadiometersA. P. Ingersoll — NASA
  16. 22webPioneer 11: Jovian Magnetic FieldM. H. Acuña — NASA
  17. 24journalSupport for the Thermal Origin of the Pioneer AnomalyS. G. Turyshev et al. — 12 June 2012
  18. 25web40 Years Ago: Pioneer 11 First to Explore SaturnJ. Uri — NASA — 3 September 2019
  19. 27journalA Message from EarthC. Sagan et al. — 25 February 1972
  20. 29webMilestones of FlightSmithsonian National Air and Space Museum
  21. 32webPioneer 11: Up Close with Jupiter & SaturnE. Howell — 26 September 2012
  22. 33webThe Pioneer MissionsNASA / Ames — 27 March 2007
  23. 35encyclopediaPioneer 119 November 2010