/* MODIFICATIONS: /* 920929 RMONARREZ /* Generated from database /* Template: Mission Template Rev: 19890121 */ /* Note: The following templates form part of a standard set */ /* for the submission of a mission to the PDS. */ /* Hierarchy: MISSION */ /* MSNINFO */ /* MSNPHSINFO */ /* MSNREFINFO */ /* REFERENCE */ /* REFAUTHORS */ OBJECT = MISSION MISSION_NAME = "VOYAGER" OBJECT = MSNINFO MISSION_START_DATE = 1972-07-01 MISSION_STOP_DATE = UNK MISSION_ALIAS_NAME = "MJS77" MISSION_DESC = " The Voyager mission was the product of a redesign of the Outer Planets grand tour conceived in the late 1960s. Direct measurement instruments on Voyager measured cosmic ray particles, low energy charged particles, magnetic fields, plasma particles and plasma waves. The remote sensing investigations were essentially astronomical in nature, measuring the lighter radio waves reflected or emitted by the planets and their satellites. A final Voyager investigation used the radio telemetry link between the spacecraft and controllers on Earth to probe the atmospheres of the planets and satellites and to determine the masses of planets and satellites as the spacecraft passed near them. The Voyager mission used two identical spacecraft. Each Voyager spacecraft followed a billion-kilometer path to Jupiter, where the gravitational pull of the giant planet was used to redirect the trajectory toward Saturn. Voyager 1 received a larger kick from the gravitational slingshot than Voyager 2, increasing its lead so that it arrived at Saturn in November 1980, about nine months before Voyager 2. During the Saturn flyby, Voyager 1s trajectory was deflected northward of the ecliptic plane, in which the solar system planets orbit. Voyager 2 used the Saturn flyby to redirect its path toward a Uranus encounter in 1986. (Refer to Morrison, 1982)" MISSION_OBJECTIVES_SUMMARY = " Voyager's objective was the exploration of the two giant planets, Jupiter and Saturn, and their magnetospheres and satellites. Major emphasis was placed on studying the satellites, many of which are planet-sized worlds, in as much detail as possible. The study of Titan, the only satellite in the solar system known to have an extensive atmosphere, was nearly as high a priority as studies of Saturn itself.(Refer to Morrison, 1982)" OBJECT = MSNPHSINFO SPACECRAFT_ID = VG2 TARGET_NAME = NEPTUNE MISSION_PHASE_TYPE = ENCOUNTER SPACECRAFT_OPERATIONS_TYPE = FLYBY MISSION_PHASE_START_TIME = 1989-06-05 MISSION_PHASE_STOP_TIME = 1989-10-02 MISSION_PHASE_DESC = " This mission phase covers all Neptune encounter science activities and includes both the observatory and close encounter periods." END_OBJECT = MSNPHSINFO OBJECT = MSNPHSINFO SPACECRAFT_ID = VG2 TARGET_NAME = URANUS MISSION_PHASE_TYPE = ENCOUNTER SPACECRAFT_OPERATIONS_TYPE = FLYBY MISSION_PHASE_START_TIME = 1985-11-04 MISSION_PHASE_STOP_TIME = 1986-02-25 MISSION_PHASE_DESC = " This mission phase covers all Uranus encounter science activities and includes both the observatory and close encounter periods." END_OBJECT = MSNPHSINFO END_OBJECT = MSNINFO OBJECT = MSNREFINFO REFERENCE_KEY_ID = "MORRISON1982" OBJECT = REFERENCE DOCUMENT_TOPIC_TYPE = "MISSION DESCRIPTION" JOURNAL_NAME = "NASA PUBLICATION" PUBLICATION_DATE = 1982 REFERENCE_DESC = " Morrison, D., Voyages to Saturn, NASA SP-451, Washington, 1982." OBJECT = REFAUTHORS AUTHOR_FULL_NAME = "DAVID MORRISON" END_OBJECT = REFAUTHORS END_OBJECT = REFERENCE END_OBJECT = MSNREFINFO END_OBJECT = MISSION