3 micron spectroscopy of comet Halley (1982i)

Details 3 micron spectroscopy of comet Halley (1982i) 3 micron spectroscopy of comet Halley (1982i)

Nov 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986apj...310l..45t&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor (ISSN 0004-637X), vol. 310, Nov. 1, 1986, p. L45-L48.

Astronomy and Astrophysics

Astrophysics

11

Comet Nuclei, Halley'S Comet, Infrared Spectroscopy, Ice, Infrared Photometry, Light Scattering, Solar Radiation, Thermal Emission, Water

Scientific paper

Near-infrared spectroscopy and photometry was obtained of comet Halley in December 1985 when its heliocentric distance was 1.19 AU. No water ice absorption or molecular band emission were observed. The interstellar 3.3-micron emission band was also not observed. The 3-micron spectrum of comet Halley consisted of scattered sunlight at wavelengths less than 3.1 microns and of thermal emission by dust at longer wavelengths.

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