NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
The 1983 June 15 occultation by Neptune. I - Limits on a possible ring systemObservations on 15 June 1983 of an occultation of a star by Neptune from Mauna Kea, Mount Stromlo, Siding Spring, and the Kuiper Airborne Observatory show no evidence for equatorial rings between 25,300 and 200,000 km (R/N/ = 25,269 km). Within most of this region, the upper limit on the optical depth along the line of sight, for rings broader than 6 km , is 0.04, which corresponds to a normal optical depth of 0.016. These results rule out a Neptunian ring system similar to that of Saturn or Uranus, but not a system of low optical depth similar to the Jovian rings. The data show no features that appear likely to have been caused by material in the equatorial plane of Neptune near the Roche limit.
Document ID
19860033532
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Elliot, J. L.
(Massachusetts Inst. of Tech. Cambridge, MA, United States)
Baron, R. L.
(Massachusetts Inst. of Tech. Cambridge, MA, United States)
Dunham, E. W.
(Massachusetts Inst. of Tech. Cambridge, MA, United States)
French, R. G.
(Massachusetts Inst. of Tech. Cambridge, MA, United States)
Meech, K. J.
(Massachusetts Inst. of Tech. Cambridge, MA, United States)
Mink, D. J.
(MIT Cambridge, MA, United States)
Erickson, E. F.
(NASA Ames Research Center Moffett Field, CA, United States)
Date Acquired
August 12, 2013
Publication Date
December 1, 1985
Publication Information
Publication: Astronomical Journal
Volume: 90
ISSN: 0004-6256
Subject Category
Astronomy
Accession Number
86A18270
Funding Number(s)
CONTRACT_GRANT: NGL-12-001-056
CONTRACT_GRANT: NSG-2342
CONTRACT_GRANT: NSF AST-82-09825
CONTRACT_GRANT: NAG7-526
Distribution Limits
Public
Copyright
Other

Available Downloads

There are no available downloads for this record.
No Preview Available