NGC 6210 has a very high
surface brightness, making it a good target for small scopes and high magnification.
Look for it between two nearly identical stars. In telescopes less than
8 inches NGC 6210 appears as a small, round, blue-green disk. Larger instruments
and/or a UHC or OIII filter may reveal a faint outer shell. On nights of
good seeing the 12.7 magnitude star should be visible at the center.
Photographs show two arcing
filaments of nebulosity to the north and south. It is unclear to me at
this time whether or not these filaments are visible in amateur instruments.
I'd love to hear from anyone who has observed them.
The view in a 6-inch
at 50x.
In April 2000 I observed
NGC 6210 with my 18-inch Dob on an excellent night under dark skies:
At 83x I was
really struck by the obvious sky-blue color. I seldom ever see color in
planetaries and when I do I usually see a very slight greenish tint. To
see blue in this one was the surprise of the night. At 430x it took on
an eerie appearance, as if it were being viewed through wrinkled cellophane,
smearing the image. It appeared as a bright oval with rough, poorly defined
edges and a very slight brightening toward the center. About this oval
I thought I could see a faint outer envelope that was slightly brighter
at the ends of the central oval.

The above image
from the DSS shows a 20' x 20' field. North is down and east is to the
right.
The above color image was
created by combining red and blue second generation sky survey images.
The odd shape of this nebula is apparent in the photograph; the appendages
are considered by some to look like the legs of a turtle. The field of
view is 5' x 5'.
At a distance of 4700 light years the apparent size of this nebula translates to an actual diameter
of about 0.4 light years or 25,000 AU. That's about 300 times larger than
our solar system if you take its diameter as the mean orbital distance
of Pluto.
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