Adaptive optics image of comet Hale-Bopp

The image shows innermost part of the comet's head. It is reproduced from an image that was obtained by Anne-Marie Lagrange, Jean Luc Beuzit and Patrice Bouchet on August 16-17, 1995, with the ADONIS adaptive optics instrument at the 3.6-metre telescope on La Silla. It is a composite of three 1-minute exposures through an infrared K-filtre centred at wavelength 2.2 microns. The field measures 13 x 13 arcseconds. The pixel size is 0.05 arcseconds. North is up and east is to the left. On this photo, the central condensation of the comet is clearly extended; it measures about 1.7 arcseconds across (FWHM), or about 7700 kilometres at the distance of the comet. It represents the densest part of the cloud of dust particles that surrounds the cometary nucleus. An asymmetric coma (dust cloud) extends towards the North.

Crédit:

ESO

À propos de l'image

Identification:eso9520b
Type:Observation
Date de publication:25 août 1995
Communiqués de presse en rapport:eso9520
Taille:509 x 513 px

À propos de l'objet

Nom:Comet Hale-Bopp
Type:Solar System : Interplanetary Body : Comet
Catégorie:Solar System

Image Formats

Grand JPEG
259,6 Kio
JPEG taille écran
525,8 Kio

Fonds d'écran

1024x768
456,5 Kio
1280x1024
649,1 Kio
1600x1200
802,8 Kio
1920x1200
843,9 Kio
2048x1536
1,1 Mio

Couleurs & filtres

DomaineLongueur d'ondeTélescope
Infrarouge
K
2.2 μmESO 3.6-metre telescope
ADONIS

Exposure time: 180s