Airborne spectrophotometry of P/Halley from 16 to 30 microns

Details Airborne spectrophotometry of P/Halley from 16 to 30 microns Airborne spectrophotometry of P/Halley from 16 to 30 microns

Dec 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986esasp.250b.117h&link_type=abstract

In ESA Proceedings of the 20th ESLAB Symposium on the Exploration of Halley's Comet. Volume 2: Dust and Nucleus p 117-120 (SEE N

Computer Science

2

Cosmic Dust, Halley'S Comet, Infrared Spectra, Spectrophotometry, Airborne Equipment, Comet Nuclei, Silicates, Space Observations (From Earth)

Scientific paper

The authors report on the first spectrum of a comet ever obtained in the 16- to 30-micron region. Comet Halley was observed using the Cornell University 7-channel spectrometer (Δλ/λ ≡ 0.02) on board the Kuiper Airborne Observatory on 1985 December 14.2. A 30-arcsec aperture (FWHM) was used. Measurements were made centered on the nuclear condensation. These observations indicate that if present, the 20 μm silicate feature is very weak, and that a relatively narrow (Δλ ≡ 0.5 μm), strong feature centered at approximately 28.4 μm possibly exists. However, this feature may be an artifact of incomplete correction for telluric water vapor absorption.

Affiliated with

Also associated with

No associations

Rating

Airborne spectrophotometry of P/Halley from 16 to 30 microns does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Airborne spectrophotometry of P/Halley from 16 to 30 microns, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Airborne spectrophotometry of P/Halley from 16 to 30 microns will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1122762