Sign on

SAO/NASA ADS Astronomy Abstract Service

· Find Similar Abstracts (with default settings below)
· Electronic Refereed Journal Article (HTML)
· Full Refereed Journal Article (PDF/Postscript)
· References in the article
· Citations to the Article (22) (Citation History)
· Refereed Citations to the Article
· Also-Read Articles (Reads History)
·
· Translate This Page
Title:
The 10 Micron Silicate Feature of Comet C/1996 Q1 (Tabur)
Authors:
Harker, David E.; Woodward, Charles E.; Wooden, Diane H.; Witteborn, Fred C.; Meyer, Alan W.
Affiliation:
AA(Wyoming Infrared Observatory, Department of Physics and Astronomy, University of Wyoming, Laramie, WY 82071-3905), AB(Wyoming Infrared Observatory, Department of Physics and Astronomy, University of Wyoming, Laramie, WY 82071-3905), AC(Space Science Division, NASA Ames Research Center, Moffet Field, CA 94035-1000), AD(Space Science Division, NASA Ames Research Center, Moffet Field, CA 94035-1000), AE(Space Science Division, NASA Ames Research Center, Moffet Field, CA 94035-1000)
Publication:
The Astronomical Journal, Volume 118, Issue 3, pp. 1423-1429. (AJ Homepage)
Publication Date:
09/1999
Origin:
AJ
AJ Keywords:
COMETS: GENERAL, COMETS: INDIVIDUAL (CSOLAR1996 Q1 (TABUR), CSOLAR1998 K5 (LINEAR)), INFRARED RADIATION
DOI:
10.1086/301011
Bibliographic Code:
1999AJ....118.1423H

Abstract

We present 7.6-13.2 μm infrared spectrophotometry (R~=120) of the inner coma of comet C/1996 Q1 (Tabur), obtained 1996 October 8-10 UT. At this epoch, the comet was at a heliocentric distance of r_h=0.96 AU. The local 10 μm continuum is fitted with a 300+/-10 K blackbody, revealing a weak silicate feature. Our analysis suggests that comet Tabur most likely contains large grains of radii a~1-3 mum. Synthetic spectra derived from laboratory measurements of amorphous pyroxene and amorphous and crystalline olivine of grain sizes (radii) between 1 and 5 μm are fitted to Tabur's silicate emission feature. A mixture of crystalline olivine (1 μm radii) and amorphous pyroxene (3 μm radii) grains provides the best model fit to the observed 10 μm spectrum. We also compare the spectra of Tabur with the mid-IR spectra of C/1995 O1 (Hale-Bopp) and other comets with and without silicate features. In particular, we discuss the mid-IR spectrum of comet C/1998 K5 (LINEAR) obtained on 1998 June 28-30 UT with the same instrument and spectral resolution. In contrast to comet Tabur, the spectrum of comet K5 LINEAR does not exhibit 10 μm silicate emission in excess of a featureless continuum characterized by a 310+/-10 K blackbody.
Bibtex entry for this abstract   Preferred format for this abstract (see Preferences)
   

Find Similar Abstracts:

Use: Authors
Title
Keywords (in text query field)
Abstract Text
Return: Query Results Return    items starting with number
Query Form
Database: Astronomy
Physics
arXiv e-prints