Comet Hale Bopp dust jets

The porcupine appearance of the multiple dust jets very much resembles the coma structures in Comet Hale-Bopp that were observed in the second half of 1996. They may also be perceived as systematic irregularities in the isophote pattern of the V-filter image. While it is therefore obvious that the dust is not at all evenly distributed throughout the coma, the gaseous coma is rather symmetric. This is most likely caused by an omni-directional expansion of the gas that is released by the nucleus. This image was obtained by Hermann Boehnhardt (ESO) and Francois Colas (Bureau des Longitudes, Paris, France) using the ESO/MPG 2.2m telescope equipped with the EFOSC2 instrument. It represents a small subset of the science data collected on comet Hale-Bopp at ESO La Silla. On the photos that are shown here, the North and East directions are inclined 12 o clockwise of the top and left edge in the images, respectively.

Crédito:

ESO

Sobre la imagen

Identificador:eso9726c
Tipo:Observación
Fecha de publicación:8 de Octubre de 1997
Noticias relacionadas:eso9726
Tamaño:671 x 677 px

Sobre el objeto

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

Formatos de imagen

JPEG grande
366,8 KB

Fondo de pantalla

1024x768
479,6 KB
1280x1024
667,7 KB
1600x1200
811,3 KB
1920x1200
837,7 KB
2048x1536
1,1 MB

Colores y filtros

BandaTelescopio
Óptico
V
MPG/ESO 2.2-metre telescope
EFOSC2