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.

Crédito:

ESO

Sobre la imagen

Identificador:eso9520b
Tipo:Observación
Fecha de publicación:25 de Agosto de 1995
Noticias relacionadas:eso9520
Tamaño:509 x 513 px

Sobre el objeto

Nombre:Comet Hale-Bopp
Tipo:Solar System : Interplanetary Body : Comet
Categoría:Solar System

Formatos de imagen

Tamaño original
775,9 KB
JPEG grande
259,6 KB

Fondo de pantalla

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

Colores y filtros

BandaLongitud de ondaTelescopio
Infrarrojo
K
2.2 μmESO 3.6-metre telescope
ADONIS

Exposure time: 180s