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The Voyager 2 encounter with the Neptunian systemAn overview of the Voyager 2 encounter with Neptune is presented, including a brief discussion of the trajectory, the planned observations, and highlights of the results described in the 11 companion papers. Neptune's blue atmosphere has storm systems reminiscent of those in Jupiter's atmosphere. An optically thin methane ice cloud exists near the 1.5-bar pressure level, and an optically thick cloud exists below 3 bars. Neptune's magnetic field is highly tilted and offset from the planet's center; it rotates with a period of 16.11 hours. Two narrow and two broad rings circle the planet; the outermost of these rings has three optically thicker arc segments. Six new moons were discovered in circular prograde orbits, all well inside Triton's retrograde orbit. Triton has a highly reflective and geologically young surface, a thin nitrogen atmosphere, and at least two active geyser-like plumes.
Document ID
19900031371
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Stone, E. C.
(California Institute of Technology Pasadena, United States)
Miner, E. D.
(JPL Pasadena, CA, United States)
Date Acquired
August 14, 2013
Publication Date
December 15, 1989
Publication Information
Publication: Science
Volume: 246
ISSN: 0036-8075
Subject Category
Lunar And Planetary Exploration
Accession Number
90A18426
Distribution Limits
Public
Copyright
Other

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