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.

Källa:

ESO

Om bilden

ID:eso9520b
Typ:Observation
Publiceringsdatum:25 augusti 1995
Relaterade pressmeddelanden:eso9520
Storlek:509 x 513 px

Om objektet

Namn:Comet Hale-Bopp
Typ:Solar System : Interplanetary Body : Comet
Kategori:Solar System

Bildformat

Originalstorlek
775,9 kB
Stor jpeg
259,6 kB
Skärmstor jpeg
525,8 kB

Skrivbordsunderlägg

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

Färger och filter

BandVåglängdTeleskop
Infrarött
K
2.2 μmESO 3.6-metre telescope
ADONIS

Exposure time: 180s