Spectroscopic study of comet Halley by the Vega 2 three-channel spectrometer

V. A. Krasnopolsky (1) , M. Gogoshev (2) , G. Moreels (3) , V. I. Moroz (1) , A. A. Krysko (1) , Ts. Gogosheva (2) , K. Palazov (2) , S. Sargoichev (2) , J. Clairemidi (3) , M. Vincent (3) , Jean-Loup Bertaux (4) , Jacques-Emile Blamont (4) , V. S. Troshin (1) , B. Valníček (5)

1 IKI - Space Research Institute of the Russian Academy of Sciences
2 Observatory Stara Zagora
3 Université de Besançon
4 SA - Service d'aéronomie
5 Ondřejov Observatory of the Prague Astronomical Institute

The three-channel spectrometer (TKS) aboard the Vega 2 spacecraft recorded infrared and visible spectra near the nucleus of comet Halley. Spectra in the range 0.95–1.9 µm at a distance of 300 km from the nucleus reveal the H2O 1.38-µm band and OH bands, the latter excited by dissociation of a parent molecule.

Domains: Instrumentation and Methods for Astrophysic [astro-ph.IM]

V. A. Krasnopolsky, M. Gogoshev, G. Moreels, V. I. Moroz, A. A. Krysko, et al.. Spectroscopic study of comet Halley by the Vega 2 three-channel spectrometer. Nature, 1986, 321 (S6067), pp.269-271. ⟨10.1038/321269a0⟩. ⟨insu-03581936⟩