Voyagers 1982 NASA JPL; Voyager 1 & Voyager 2; Jupiter & Saturn
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Voyager 1 and
Voyager 2 were launched in
1977. Both probes flew past
Jupiter and
Saturn; Voyager 2 also encountered
Uranus and
Neptune (after this film was made). The
Voyagers have left the solar system, and are expected to continue to transmit back data about extrasolar space until approximately
2020 (when their power will drop below a usable level) on the "
Voyager Interstellar Mission."
Reupload of a previously uploaded film, in one piece instead of multiple parts, and with improved sound.
Public domain video from the
National Archives with the aspect ratio corrected and mild noise reduction applied.
The soundtrack was also processed with volume normalization, noise reduction, clipping reduction, and/or equalization (the resulting sound, though not perfect, is far less noisy than the original).
History Of
The Voyager Mission (as of
October 18,
2010)
http://voyager.jpl.nasa.gov/science/planetary.html
The Voyager mission was designed to take advantage of a rare geometric arrangement of the outer planets in the late
1970s and the
1980s which allowed for a four-planet tour for a minimum of propellant and trip time. This layout of Jupiter, Saturn, Uranus and Neptune, which occurs about every
175 years, allows a spacecraft on a particular flight path to swing from one planet to the next without the need for large onboard propulsion systems. The flyby of each planet bends the spacecraft's flight path and increases its velocity enough to deliver it to the next destination. Using this "gravity assist" technique, first demonstrated with
NASA's
Mariner 10 Venus/
Mercury mission in 1973-74, the flight time to Neptune was reduced from 30 years to 12.
While the four-planet mission was known to be possible, it was deemed to be too expensive to build a spacecraft that could go the distance, carry the instruments needed and last long enough to accomplish such a long mission. Thus, the Voyagers were funded to conduct intensive flyby studies of Jupiter and Saturn only. More than 10,
000 trajectories were studied before choosing the two that would allow close flybys of Jupiter and its large moon Io, and Saturn and its large moon
Titan; the chosen flight path for Voyager 2 also preserved the option to continue on to Uranus and Neptune.
From the NASA
Kennedy Space Center at
Cape Canaveral, Florida, Voyager 2 was launched first, on August 20, 1977; Voyager 1 was launched on a faster, shorter trajectory on
September 5, 1977. Both spacecraft were delivered to space aboard Titan-Centaur expendable rockets.
The prime
Voyager mission to Jupiter and Saturn brought Voyager 1 to Jupiter on March 5,
1979, and Saturn on
November 12,
1980, followed by Voyager 2 to Jupiter on July 9, 1979, and Saturn on August 25,
1981.
Voyager 1's trajectory, designed to send the spacecraft closely past the large moon Titan and behind
Saturn's rings, bent the spacecraft's path inexorably northward out of the ecliptic plane -- the plane in which most of the planets orbit the Sun. Voyager 2 was aimed to fly by Saturn at a
point that would automatically send the spacecraft in the direction of Uranus.
After Voyager 2's successful Saturn encounter, it was shown that Voyager 2 would likely be able to fly on to Uranus with all instruments operating. NASA provided additional funding to continue operating the two spacecraft and authorized
JPL to conduct a Uranus flyby. Subsequently, NASA also authorized the Neptune leg of the mission, which was renamed the Voyager Neptune
Interstellar Mission.
Voyager 2 encountered Uranus on
January 24,
1986, returning detailed photos and other data on the planet, its moons, magnetic field and dark rings. Voyager 1, meanwhile, continues to press outward, conducting studies of interplanetary space.
Eventually, its instruments may be the first of any spacecraft to sense the heliopause -- the boundary between the end of the Sun's magnetic influence and the beginning of interstellar space.
Following Voyager 2's closest approach to Neptune on August 25,
1989, the spacecraft flew southward, below the ecliptic plane and onto a course that will take it, too, to interstellar space. Reflecting the Voyagers' new transplanetary destinations, the project is now known as the Voyager Interstellar Mission.
Voyager 1 has crossed into the heliosheath and is leaving the solar system, rising above the ecliptic plane at an angle of about 35 degrees at a rate of about 520 million kilometers (about 320 million miles) a year. Voyager 2 is also headed out of the solar system, diving below the ecliptic plane at an angle of about 48 degrees and a rate of about 470 million kilometers (about 290 million miles) a year.
Both spacecraft will continue to study ultraviolet sources among the stars, and the fields and particles instruments aboard the Voyagers will continue to explore the boundary between the Sun'
s influence and interstellar space
...