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Occultation determination of Neptune's oblateness and stratospheric methane mixing ratioThe occultation of a star by Neptune on August 20, 1985 was observed at 2.2 micron wavelength with telescopes at the European Southern Observatory (ESO) and the Cerro Tololo Inter-American Observatory (CTIO). The detection of a 'central flash' midway between immersion and emersion has allowed the determination of Neptune's oblateness and the atmospheric extinction at 2.2 microns, which is related to the stratospheric methane mixing ratio. An oblateness of (2.08 +0.19 or -0.18) x 10 to the 2nd is found and, assuming a stratospheric temperature of 120 K, a value of 0.6 percent is inferred (with an uncertainty of a factor of 10) for the methane mixing ratio (CH4/H2) at 0.3 mbar. The latter value may indicate supersaturation of methane in Neptune's stratosphere.
Document ID
19870038357
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Lellouch, E.
(Meudon Observatoire, France)
Hubbard, W. B.
(Arizona, University Tucson, United States)
Sicardy, B.
(Meudon, Observatoire; Paris VII, Universite Paris, France)
Vilas, F.
(NASA Johnson Space Flight Center Houston, TX, United States)
Bouchet, P.
(European Southern Observatory La Silla, Chile)
Date Acquired
August 13, 2013
Publication Date
November 20, 1986
Publication Information
Publication: Nature
Volume: 324
ISSN: 0028-0836
Subject Category
Lunar And Planetary Exploration
Accession Number
87A25631
Funding Number(s)
CONTRACT_GRANT: NSF AST-78-27879
CONTRACT_GRANT: NSG-7045
Distribution Limits
Public
Copyright
Other

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