Stellar cluster and star-forming region M 17 (annotated)

Three-colour composite of the sky region of M 17, a H II region excited by a cluster of young, hot stars. A large silhouette disc has been found to the south-west of the cluster centre. The present image was obtained with the ISAAC near-infrared instrument at the 8.2-m VLT ANTU telescope at Paranal. The orientation and the scale at the distance of M 17 (7,000 light-years) are indicated, and the main regions are identified.

Kilde:

ESO

Om billedet

Id:eso0416b
Type:Observation
Udgivelsesdato:12. maj 2004
Relaterede pressemeddelelser:eso0416
Størrelse:773 x 772 px

Om objektet

Navn:Messier 17, Omega Nebula
Type:Milky Way : Nebula : Appearance : Emission : H II Region
Milky Way : Nebula : Type : Star Formation
Afstand:5500 lysår
Constellation:Sagittarius
Kategori:Star Clusters

Billedformater

Stor JPEG
270,6 KB
Skrærm JPEG
315,5 KB

Baggrundsbilleder

1024x768
317,4 KB
1280x1024
442,6 KB
1600x1200
554,9 KB
1920x1200
596,0 KB
2048x1536
751,5 KB

Koordinater

Position (RA):18 20 47.06
Position (Dec):-16° 10' 19.25"
Field of view:6.03 x 6.02 arcminutes
Orientering:Nord er 0.1° venstre fra lodret

Farver & filtre

BåndBølgelængdeTeleskop
Infrarød
J
1.25 μmVery Large Telescope
ISAAC
Infrarød
H
1.6 μmVery Large Telescope
ISAAC
Infrarød
K
2.2 μmVery Large Telescope
ISAAC