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Messier 66
Spiral Galaxy
M66 (NGC 3627), type Sb, in
Leo
in the Leo Triplett
| Right Ascension |
11 : 20.2 (h:m)
|
| Declination |
+12 : 59 (deg:m)
|
| Distance |
35000 (kly)
|
| Visual Brightness |
8.9 (mag)
|
| Apparent Dimension |
8x2.5 (arc min)
|
Discovered 1780 by Charles Messier.
Messier 66 (M66, NGC 3627), together with its neighbors
M65 and
NGC 3628,
forms a most conspicuous triplet of galaxies, the
Leo Triplett or
M66 group, located at a distance of about 35 million light years.
M66 is considerably larger than its neighbor,
M65, and has a
well developed but not well defined central bulge, and is therefore
classified Sb. Obviously its spiral arms are deformed, probably because of
the encounters with its neighbors. They seem to be distorted and displaced
above the plane of the galaxy. Note how one of the spiral arms seems to pass
over the left side of the central bulge. Much dust is visible here, as well
as a few pink nebulae, signs of star formation, near the end of one of the
arms.
This image was obtained by
David Malin
with the 3.9-meter Anglo Australian
Telescope; interested readers may obtain
more
detailed information on this image.
Together with its neighbor M65, M66 has been discovered by
Charles Messier, who
cataloged it on March 1, 1780, remarks that he missed these two objects
in 1773, when a comet passed between them on November 1 to 2, 1773, probably
because of the light of the comet. Because of a dubious error,
Admiral
Smyth has
assigned this discovery of M65 and M66 (and
M68) to
Pierre Méchain, a view which was adopted by
Kenneth Glyn
Jones somewhen in the 1960s, and consequently, in many modern sources,
despite the fact that Messier doesn't acknowledge such a prior sighting,
which he did in all other cases.
Three supernovae have appeared in this galaxy:
- 1973R which was of type II and reached mag 15 was found on Dec 12,
1973.
-
1989B was discovered on Jan 31, 1989 and became as bright as mag
12.2 on Feb 1, 1989.
-
1997bs was discovered by the Lick Observatory Supernova Search Team
as it occurred on April 15, 1997 at 13" west, 67" south of the galaxy's
center and reached mag 17.0; this was of peculiar type IIn.
Halton Arp has included M66 in his
Catalogue
of Peculiar Galaxies as entry No. 16. Moreover, he assigned the number
317 to the Leo Triplett (M66 together with M65 and NGC 3628).
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