Infrared observations of P/Halley and P/Encke

Details Infrared observations of P/Halley and P/Encke Infrared observations of P/Halley and P/Encke

Sep 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988ioch.rept..145g&link_type=abstract

In NASA, Washington, Infrared Observations of Comets Halley and Wilson and Properties of the Grains p 145-146 (SEE N89-13330 04-

Astronomy and Astrophysics

Astronomy

Astronomical Photometry, Cosmic Dust, Encke Comet, Halley'S Comet, Infrared Spectra, Comet Tails, Emission Spectra, Grain Size, Silicates, Spectral Energy Distribution, Spectrum Analysis

Scientific paper

Broadband optical/infrared photometers responding from 0.5 to 23 microns mounted on the Univ. of Minnesota (UM) O'Brien 76-cm telescope, Wyoming Infrared Observatory 234-cm telescope, and UM's Mount Lemmon Infrared Observatory 152-cm telescope were used to measure comet Halley more than 30 times between 12 Dec. 1985 to 6 May 1986. The Wyoming system was used to measure P/Encke on 24 Jul. 1987. The equipment and observations of Halley were fully described by Gehrz and Ney. Conclusions based on a preliminary analysis of the Halley and P/Encke data are reported.

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