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The Trifid Nebula. Photo: Mike Selby.
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Trifid Nebula annotated.
What a beautiful APOD!
Here are a few annotations:
1)
HD 164492, spectral class O7.5V, ionizing star of the Trifid Nebula. It is the brightest of
a small grouping of stars, of which
one is supposed to be an evolved supergiant star! Really...?
2) Dust pillar close to the small group of hot stars. Note that the dust pillar has a bright rim. It is directly illuminated by the stars.
3) Small jet protruding from a fat dust pillar. The jet has been emitted by a newborn star. Actually there are
two jets!
4) HD 164514, an evolved supergiant star of spectral class A7Iab/b. Note the yellow color of this star, whose intrinsic color is probably as white as that of Summer Triangle star
Altair. This star is the probable source of the blue reflection nebula surrounding the Trifid, and the star's own yellow color testifies to the fact that much of its blue light has been scattered by dust.
5) "Foreground dust" darkening and reddening the blue reflection nebula to a greenish gray color.
Cocoon Nebula Marcel Drechsler.png
Very deep view of the Cocoon Nebula. Photo: Marcel Drechsler.
The Trifid Nebula shows some similarities with the Cocoon Nebula. Many images show the Cocoon Nebula to be "all red", but many also show a faint outer blue rim around it. The very deep image of the Cocoon that I have posted here shows a very large blue reflection nebula surrounding the Cocoon. This reflection nebula is really there, but it is very faint.
My point is that the blue reflection nebula of the Trifid Nebula is not exclusively the product of the yellow-looking reddened A-type supergiant star immediately to the north of the Trifid. Instead, we should think of the small grouping of stars in the center of the Trifid as providing not only the ultraviolet light needed to ionize the red lobes of the Trifid, but also contributing significantly to the blue light surrounding this famous nebula.
Ann
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