Star cluster RCW 38

The dense star cluster RCW 38 glistens about 5,500 light years away in the direction of the constellation Vela (the Sails). RCW 38 is an "embedded" cluster, in that the nascent cloud of dust and gas still envelops its stars. There, young, titanic stars bombard fledgling suns and planets with powerful winds and large amount of light, helped in their devastating task by short-lived, massive stars that explode as supernovae. In some cases, this energetic onslaught cooks away the matter that may eventually form new planetary systems. Scientists think that our own Solar System emerged from such a dramatic environment.

This image was obtained with the Wide Field Imager instrument on the MPG/ESO 2.2-metre telescope at La Silla, using data collected through four filters (B, V, R and H-alpha). The field of view is about 10 arcminutes.

Credit:

ESO

Over de afbeelding

Id:eso0929b
Type:Observatie
Publicatiedatum:19 augustus 2009
Gerelateerde berichten:eso0929
Grootte:2946 x 2944 px

Over het object

Naam:RCW 38
Type:Milky Way : Star : Grouping : Cluster
Afstand:5500 lichtjaren
Constellation:Vela
Categorie:Star Clusters

Afbeeldingstypen

Grote JPEG
1,5 MB

Inzoomen


Achtergrond

1024x768
245,9 KB
1280x1024
369,9 KB
1600x1200
488,3 KB
1920x1200
539,1 KB
2048x1536
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Coordinates

Position (RA):8 59 7.92
Position (Dec):-47° 31' 45.78"
Field of view:11.68 x 11.67 arcminutes
Orientation:North is 1.6° right of vertical

Kleuren & filters

BandTelescoop
Optisch
B
MPG/ESO 2.2-metre telescope
WFI
Optisch
Pseudogreen (B+R)
MPG/ESO 2.2-metre telescope
WFI
Optisch
H-alpha
MPG/ESO 2.2-metre telescope
WFI
Optisch
R
MPG/ESO 2.2-metre telescope
WFI