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Gum 31 - a part of NGC 3372 -the large Eta Carinae
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Description of
object:
The emission nebula
Gum 31 can be found directly northwest of the well-known Eta Carinae Nebula and
is usually visible just on the edge within overview pictures of the region.
This interesting nebula bubble is ionized by the hot stars of the star cluster
NGC 3324, slightly to the right of the nebulas center.
The brightest
star in the picture, HD 92207, is a supergiant of the spectral class A with a
mass of almost 30 sun masses. HD 92207 is located in a nebula shell of Gum 31
which is most probably responsible for the blue reflection part directly south
(left in the picture) of the star. Its temperature however is not high enough
to ionize the gas nebula.
The distance to Gum 31 is being declared as
7500 light years. With an apparent diameter of 15 arc minutes in the sky the
absolute diameter is 30 light years. The visible field of view equates to about
the size of the area of the half moon. |
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The
picture on the left shows the position of GUM 31 within the Eta Carina complex.
It is a mosaic of 5 segments and was also shot in Rooisand in 2009. The
telescope used was a 6'' Zeiss APQ with AP Reducer at f = 900mm.
« Load the high-res picture (2200 x 1500
Pixel). Additional picture information available
here.
A detailed shot of the lower right edge of the nebula bubble was made
by the Hubble space telescope and
is available here |
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