Identification of Polycyclic Aromatic Molecules in the UV Spectrum of Comet P/Halley

Published

Journal Article

Emission spectra of comet P/Hallev in the 275–710 nm wavelength range were obtained by using a spectrometer carried on board the Vega 2 spacecraft which encountered the famous comet on March 9, 1986. The spectrum, after subtraction of the intense solar continuum, shows the presence of two new spectral features: An isolated band at 323 nm and a broad band with four peaks at 347, 356, 364 and 374 nm. We compared our cometary spectra with UV laboratory spectra of polycyclic aromatic hydrocarbons having 2 and 3 benzenoid rings. We can securely propose the identification of phenanthrene and suggest the presence of naphthalene in Halley's comet. © 1995, Taylor & Francis Group, LLC. All rights reserved.

Full Text

Duke Authors

Cited Authors

  • Moreels, G; Clairemidi, J; Rousselot, P; Goidet, B; Vo-Dinh, T

Published Date

  • July 1, 1995

Published In

Volume / Issue

  • 5 / 1-4

Start / End Page

  • 107 - 114

Electronic International Standard Serial Number (EISSN)

  • 1563-5333

International Standard Serial Number (ISSN)

  • 1040-6638

Digital Object Identifier (DOI)

  • 10.1080/10406639408015161

Citation Source

  • Scopus