Infrared/visible comparison of the full VISTA Orion Nebula image

The left-hand panel shows the Orion Nebula in visible light. Most of the light from the spectacular clouds comes from hydrogen gas glowing under the fierce ultraviolet glare from the central hot young stars. The region above the centre is clearly obscured by dust clouds. On the right the VISTA infrared view is shown. By observing infrared light many new features appear, including large numbers of young stars close to the centre and many curious red objects, associated with young stars and their outflows, in the region above the centre.

Källa:

ESO/J. Emerson/VISTA & R. Gendler. Acknowledgment: Cambridge Astronomical Survey Unit

Om bilden

ID:eso1006c
Typ:Observation
Publiceringsdatum:10 februari 2010 12:00
Relaterade pressmeddelanden:eso1006
Storlek:6000 x 4000 px

Om objektet

Namn:Messier 42, Orion Nebula
Typ:Milky Way : Nebula : Type : Star Formation
Avstånd:1400 ljusår
Kategori:Nebulae

Bildformat

Originalstorlek
27,7 MB
Stor jpeg
4,5 MB
Skärmstor jpeg
210,9 kB

Zoombar


Skrivbordsunderlägg

1024x768
288,3 kB
1280x1024
448,8 kB
1600x1200
619,0 kB
1920x1200
743,4 kB
2048x1536
936,4 kB

Färger och filter

BandTeleskop
Infrarött
Z
Visible and Infrared Survey Telescope for Astronomy
VIRCAM
Infrarött
J
Visible and Infrared Survey Telescope for Astronomy
VIRCAM
Infrarött
K
Visible and Infrared Survey Telescope for Astronomy
VIRCAM

Noter: VISTA data relates to the right image. Optical image by Rob Gendler.