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Activities of the Department of Astronomy and McDonald Observatory of the University of Texas at AustinMcDonald Observatory of the University of Texas at Austin reports on its activities during the period 1 Jan. 1986 to 30 June 1986. Extensive observations of Halley's Comet were obtained. The comet exhibited large variability; moreover, its variability was much more rapid than can be accounted for by water vaporization as the sole controller of activity. Jupiter satellite Io's atmosphere was found to be distended by more than the equilibrium scale height but less than for unimpeded streaming into space. The atmosphere is at least temporarily bound to IO. Uranus' (3-0) H2 quadrupole line shapes require a modification of Baines and Bergstralh's standard model which incorporates at high altitude absorbing haze in addition to the lower haze layer. A fraction of normal H2 equal to 0.25 + or 0.10 is derived, in good agreement with the standard model. This result is unchanged when the preliminary temperature structure derived by the Voyager Radio Occultation Experiment is used instead of Appleby's model c. Out of the six Pluto-Charon mutual events observed this year, data were obtained on four. Preliminary analysis is yielding improved estimates for the diameters, masses, densities, and albedos of these objects.
Document ID
19860022906
Acquisition Source
Legacy CDMS
Document Type
Contractor Report (CR)
Authors
Smith, H. J.
(Texas Univ. Austin, TX, United States)
Date Acquired
September 5, 2013
Publication Date
January 1, 1986
Subject Category
Astronomy
Report/Patent Number
SAR-25
NAS 1.26:179667
NASA-CR-179667
Report Number: SAR-25
Report Number: NAS 1.26:179667
Report Number: NASA-CR-179667
Accession Number
86N32378
Funding Number(s)
CONTRACT_GRANT: NGR-44-012-152
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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