Optical spectroscopy of comet C/1995 O1 Hale-Bopp

A. Fitzsimmons*, I. M. Cartwright

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

21 Citations (Scopus)


We report the results of optical CCD spectroscopy of comet C/1995 O1 Hale-Bopp on 1995 August 30, when the comet was at a heliocentric distance of Rh = 6.82 au. In the wavelength range 3300 to 5500 Å the dust coma is found to be red compared with solar colours. Near the nucleus and in the prominent jet observed at this time the dust is redder than in the surrounding coma, implying differences between the grain populations in these regions. Emission from the CN (0-0) band was detected at a level of (1.7±0.8) × 10-14 erg s-1 cm-2. This is the first reported optical detection of gas molecules in the coma. Monte Carlo modelling gives an outgassing rate of Q(CN) = (6 ±3) × 1025 molecule s-1 at this time. From a comparison of these and other reported observations, Hale-Bopp appears to be a normal comet, albeit highly active.

Original languageEnglish
JournalMonthly Notices of the Royal Astronomical Society
Issue number2
Publication statusPublished - 01 Jan 1996


  • Comets: individual: Hale-Bopp

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science


Dive into the research topics of 'Optical spectroscopy of comet C/1995 O1 Hale-Bopp'. Together they form a unique fingerprint.

Cite this