At first glance the 9th magnitude central star of this planetary nebula
all but drowns out the surrounding nebulosity. This is particularly
true on those cold winter nights when Taurus is high in the sky and the bright stars take on halos.
The roundish glow surrounding this star can look like just another halo.
Because it can be so easily overlooked the trick to finding this one is
to first identify the 9th magnitude central star. This star is the center
of three 9th magnitude stars that make a nearly straight line. These three
stars are obvious at low power.
It is when the magnification is increased that the
nebula becomes more apparent. In my 6-inch I could make out a round
glow at 133x. I found the best view in my 18-inch to be at 166x, where
a very faint haze with hints of structure can be glimpsed without a filter.
An OIII or UHC filter really brings this one out. With the OIII in place
a dark center appeared and blotchy markings could be glimpsed in the surrounding,
fairly round, nebula. The markings are no doubt the dark patches
seen in the image at the right.
In even larger instruments the nebula is said to appear
box shaped and a faint outer envelope appears. The structure seen
in photographs is readily apparent.
The view in a 6 inch at 50X. North is down and
east is to the right.
William Herschel wrote of this nebula:
A most singular phenomenon! A star of
about 8th magnitude with a faint luminous atmosphere, of circular form,
and about 3 minutes in diameter. The star is in the centre, and the
atmosphere is so faint and delicate and equal throughout that there can
be no surmise of its consisting of stars; nor can there be a doubt of the
evident connection between the atmosphere and the star.
At the time it was commonly assumed that all nebulae were
swarms of faint stars that were unresolved; something that is true of many
objects such as galaxies. NGC 1514 and a few other planetary nebulae
gave Herschel some pause concerning this assumption. |