NGC 6751 () is a 12.5
magnitude, 10" diameter planetary nebula that gained fame recently as a
target of the Hubble Space Telescope. NGC 6751 surrounds a 15.4 magnitude
central star and lies about 8000 light years distant. In the eyepiece it
looks like a tiny version of the famous Ring Nebula.
The above HST
image shows the fine structure of this nebula. It won't look like this
in the eyepiece of course, but the irregular brighter edge can be glimpsed
if you look for it.
At low magnification it may
at first look starlike, although the star may appear obviously "wrong"
somehow. Once you have found the right location, it is important
to use high magnification on this small, egg-shaped nebula. It seems to
me that the central star is considerably brighter than the 15th magnitude
listed. Six to eight inch scopes will show a small egg. Larger scopes will
reveal a dark center giving it the appearance of a tiny, faint Ring nebula.
Users of larger scopes should also look for the central star.
This is the view of the
field in a 6-inch at 50x.
In May 2000 I observed NGC
6751 with my 18-inch f/4.5 Dob:
This is a 12.5
magnitude planetary 20" in diameter. It was obvious at 81x, even though
small. The best view came with the 4.8mm Nagler coupled to a 2X barlow
(850x). It looked like a small ring nebula surrounding a 15th magnitude
star. It seemed to me that the inner portions surrounding the star were
darker. This one is small but nice. I liked it.

This image is from
the first generation DSS and shows a 5' x 5' field. North is down and east
is to the right.
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