ThePioneer programs were two series ofUnited States lunar and planetaryspace probes. The first program, which ran from 1958 to 1960, unsuccessfully attempted to send spacecraft to orbit the Moon, successfully sent one spacecraft to fly by the Moon, and successfully sent one spacecraft to investigate interplanetary space between the orbits of Earth and Venus. The second program, which ran from 1965 to 1992, sent four spacecraft to measure interplanetaryspace weather, two to exploreJupiter andSaturn, and two to exploreVenus. The two outer planet probes,Pioneer 10 andPioneer 11, became the first two offive artificial objects to achieve theescape velocity that will allow them toleave the Solar System, and carrieda golden plaque each depicting a man and a woman and information about the origin and the creators of the probes, in case anyextraterrestrials find them someday.
Credit for naming the first probe has been attributed to Stephen A. Saliga, who had been assigned to the Air Force Orientation Group, Wright-Patterson AFB, as chief designer of Air Force exhibits. While he was at a briefing, the spacecraft was described to him, as, a "lunar-orbiting vehicle, with an infrared scanning device." Saliga thought the title too long, and lacked theme for an exhibit design. He suggested, "Pioneer", as the name of the probe, since "the Army had already launched and orbited the Explorer satellite, and their Public Information Office was identifying the Army, as, 'Pioneers in Space,'" and, by adopting the name, the Air Force would "make a 'quantum jump' as to who, really, [were] the 'Pioneers' in space.'"[1]
The earliest missions were attempts to achieve Earth'sescape velocity, simply to show it was feasible and to study theMoon. This included the first launch byNASA which was formed from the oldNACA. These missions were carried out by theAir Force Ballistic Missile Division,Army, and NASA.[2]
Five years after the early Able space probe missions ended,NASA Ames Research Center used the Pioneer name for a new series of missions, initially aimed at theinner Solar System, before the flyby missions toJupiter andSaturn. While successful, the missions returned much poorer images than theVoyager program probes would five years later. In 1978, the end of the program saw a return to the inner Solar System, with thePioneer Venus Orbiter andMultiprobe, this time using orbital insertion rather than flyby missions.
The new missions were numbered beginning with Pioneer 6 (alternate names in parentheses).
Pioneer 9 (Pioneer D) – launched November 1968 (inactive since 1983)
Pioneer E – lost in launcher failure August 1969
Pioneer 6 and Pioneer 9 are in solar orbits with 0.8AU distance to the Sun. Their orbital periods are therefore slightly shorter than Earth's. Pioneer 7 and Pioneer 8 are in solar orbits with 1.1 AU distance to the Sun. Their orbital periods are therefore slightly longer than Earth's. Since the probes' orbital periods differ from that of the Earth, from time to time, they face a side of the Sun that cannot be seen from Earth. The probes can sense parts of the Sun several days before the Sun's rotation reveals it to ground-based Earth orbiting observatories.
Map showing location and trajectories of thePioneer 10 (blue),Pioneer 11 (green),Voyager 1 (purple) andVoyager 2 (red) spacecraft, as of April 4, 2007ThePioneer plaque attached to Pioneers10 and11