Globular Clusters - Winter and Spring
NGC4147 in Coma Berenices
Magnitude 10.3 - Diameter 4.1' - class. VI
Lum: 22 Apr 2007 - C8 @ f/6.3 - SXV-H9
L = 32 min (poor and deteriorating transparancy)
A pretty unknown globular cluster located at the outskirts of the Virgo Cluster
M3 (NGC 5272) in Canes Venatici
Magnitude 6.3 - Diameter 18.0' - class. VI
Lum: 17 May 2004 - C8 @ f/6.3 - SXV-H9
RGB: 08 Jun 2005 - C8 @ f/6.3 - SXV-H9 and SXV guider
LRGB = 25:18:18:18 min
Together with M53 and M5 the prelude to the summer display of globular clusters.
Full resolution (1344 x 997)
Old MX516 image
M53 (NGC 5024) in Coma Berenices
Magnitude 7.7 - Diameter 13.0' - class. V
30 Apr 2005 - C8 at f/6.3 - SXV-H9 - SXV Guider
L = 50 min (25 x 120 sec)
First success with the SXV autoguider and Celestron Radial Guider
Full resolution (1226 x 984)
Old MX516 image
NGC 5466 in Boötes (and C/2003 K4 (LINEAR))
Magnitude 9.2 - Size 9.0' - class. XII
28 Jul 2004, 21:30 UT - C8 at f/6.3 - SXV-H9
L = 17 x 60 sec
NGC 5466 is, like NGC 5053, one of the more pathetic globulars.
So, to make it slightly more interesting I waited until comet 2003 K4 passed along :-)
Note the little galaxy, PGC 50187, to the right of the comet.
NGC 2419, The Intergalactic Wanderer in Lynx
Magnitude 10.4 - Size 6.2'
2003 Dec 17 - C8 @ f/6.3 - SXV-H9
L = 15 min binned 1x1
NGC 2419 is a very distant globular 300000 light years away. It got its nickname because it
has long been suspected that it was not gravitationally bound to our galaxy, in fact it is.
Despite the great distance it is comparably easy to observe as it is one of the intrinsically
brightest globular clusters of our Milky Way. Two 7th magnitude stars to the west of the
cluster make it easy to locate the cluster. One of those stars is visible here. This is the only readily
available winter globular from my location. M79 south of Orion is too low.
NGC5053 in Coma Berenices
Magnitude 9.0 - Diameter 10.0' - class. XI
13 Apr 2001 - C8 at f/6.3 - MX516
L = 12.5 minutes (25 x 30 sec)
This sparse globular is located just one degree from M53. It looks more like an
open cluster to me.
All images © Ole Nielsen 1999-2007