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Spectroscopic Evidence of Organic Molecules Released By the Dust of Halley’s Inner Coma

Published online by Cambridge University Press:  12 April 2016

J. Clairemidi ,
P. Rousselot  and
G. Moreels
J. Clairemidi
Affiliation:
Observatoire de Besangon BP 1615 25010 Besancon CedexFrance
P. Rousselot
Affiliation:
Observatoire de Besangon BP 1615 25010 Besancon CedexFrance
G. Moreels
Affiliation:
Observatoire de Besangon BP 1615 25010 Besancon CedexFrance

Abstract

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New spectroscopic arguments supporting the probable presence of organic molecules in the material released by comet Halley are deduced from the data obtained by the Vega three-channel spectrometer. Two excesses of emission on the UV side of the OH and CN bands at 305 and 383 nm are interpreted as being due to “prompt” radiation emitted by electronically excited OH and CN radicals directly produced by the photolysis of water vapor and an organic X-CN molecule. A broad-band emission progressively appears between 342 and 375 nm when the solar scattered continuum has been substracted. This emission increases approximately as the inverse of the projected distance to the nucleus. It is interpreted as a fluorescence emission of organic molecules, possibly condensed polycyclic hydrocarbons. Present observations support the hypothesis of grains coated with organic material and give arguments in favor of a probable interstellar origin for cometary dust.

Type
Cometary Dust: Observations and Evolution
Information
International Astronomical Union Colloquium , Volume 126: Origin and Evolution of Interplanetary Dust , 1991 , pp. 217 - 220
Copyright
Copyright © Kluwer 1991

References

Baas, F., Geballe, T.R., Walther, D.M. (1986), Astrophys. J., 311, L97–L101 Google Scholar
Clairemidi, J., Moreels, G., Krasnopolsky, V.A. (1990), Astron. Astrophys.., 221, 235–240 Google Scholar
Clairemidi, J., Brandon, E., Rousselot, P., Moreels, G., This volume, Paper P-50, 4 pagesGoogle Scholar
Combes, M., et al. (1988), Icarus, 76, 404–436 Google Scholar
Danks, A.C., Encrenaz, T., Bouchet, P., Le Bertre, T., Chalabaev, A. (1987), Astron. Astrophys., 184. 329–332 Google Scholar
Encrenaz, T., Knacke, R.F., Crovisier, J. (1989), Bull. Amer. Astron. Soc., 21, 3 Google Scholar
Greenberg, J.M. (1982) in Comets, Univ. Arizona Press, 131–163 Google Scholar
Greenberg, J.M., Hage, (1990), Astrophys. J. 361 260–274 Google Scholar
Jessberger, E.K., Christoforidis, A., Kissel, J. (1988), Nature, 332, 691–695 Google Scholar
Kissel, J. et al. (1986), Nature, 221, 280–282 CrossRefGoogle Scholar
Shafizadeh, N.. Rostas, J., Lemaire, J.L., Rostas, F. (1988), Chem. Phys. Letters, 152,11, 75–80 Google Scholar