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Impact of Saturn ring particles on Pioneer 11The detection of particles near the rings of Saturn by the meteoroid detection instrument on board Pioneer 11 is discussed. The instrument consists of 234 penetration detectors, distributed between two independent data channels each of which is designed to become inhibited for a period of 77 min after the registration of a penetration event in that channel. At least four particles penetrated the detectors in the 4.5 h period around Saturn periapsis at radial distances between 1.36 and 3.1 Saturn radii, a radial distribution inconsistent with the gravitational focusing of meteoroids. The detection of particles which may have been part of the E ring before the crossing of the ring plane suggests that this ring may be 1800 km thick, with an optical thickness greater than 10 to the -8th.
Document ID
19800034955
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Humes, D. H.
(NASA Langley Research Center Hampton, VA, United States)
Oneal, R. L.
(NASA Langley Research Center Hampton, VA, United States)
Kinard, W. H.
(NASA Langley Research Center Hampton, VA, United States)
Alvarez, J. M.
(NASA Langley Research Center Hampton, Va., United States)
Date Acquired
August 10, 2013
Publication Date
January 25, 1980
Publication Information
Publication: Science
Volume: 207
Subject Category
Lunar And Planetary Exploration
Accession Number
80A19125
Distribution Limits
Public
Copyright
Other

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