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NGC 6231, the dark cloud Sandqvist 19 and Zeta 1+2
Scorpii |
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Description of
object:
The open star cluster
NGC 6231 can already be seen with the naked eye next to the bright star zeta
Scorpii in the constellation Scorpio. The cluster belongs to a larger group of
young and hot stars known as the Scorpius OB I Association. The distance to NGC
6231 is about 5700 light years. With a diameter of 15 arcminutes in the sky,
the absolute diameter of the brightest part of the cluster is 25
lightyears.
Zeta Scorpii consists
of two stars, which however form only one optical double star system. The
brighter component, Zeta 2 Scorpii, is an ordinary orange giant star 150
light-years away.
The apparently
slightly fainter component Zeta 1 Scorpii is one of the most luminous stars in
the Milky Way and is nearly 40 times as far away. It belongs to the Scorpius OB
I association and possibly also to the star cluster NGC 6231, which is about 1
million times more luminous, 60 times more massive than our Sun and belongs to
the class of hypergiants, which includes the most massive and luminous stars in
existence. |
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NGC
6231 and Zeta1 Scorpii are equally affected by interstellar dust. It attenuates
the light of the stars by at least a factor of 6 and also leads to a reddening
of the starlight. This is why the young, hot stars of the cluster and Zeta1
Scorpii do not appear particularly blue, but rather whitish, since the blue
part is scattered out in the interstellar dust.
In the left half of the
image the very dense dark cloud Sandqvist 19 appears as a dark spot in front of
the Milky Way background. Next to it is a brighter piece of emission nebula,
which covers the whole region in Scorpio.
« In the
labeled version, the cluster can be compared with the size of the moon. To load
the large version
click here or on the preview image.
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