Palomar 2

Globular Cluster Palomar 2, class IX, in Auriga

[Palomar 2, C&D Schur]

RA:
04:46:05.91
Dec:
+31:22:53.4
Distance from Sun:
88.7 kly
Distance from Galactic Center:
114.1 kly
Apparent Diameter:
1.9 arc min
Brightness:
13.04 mag vis
Radial Velocity:
-133.0 +/- 57.0 km/s
Diameter:
ly
Abs. Mag:
-7.97 Mag vis
Discovered by A.G. Wilson in 1955.

This cluster is perhaps a former member of the Sagittarius Dwarf Elliptical Galaxy (SagDEG), or Sagittarius Dwarf Spheroidal Galaxy (Sgr dSph), the nearby dwarf galaxy discovered in 1994, which is currently in a close and perhaps final encounter before its tidal disruption, with our Milky Way Galaxy.

The image on the right was obtained by Chris and Dawn Schur from Payson, Arizona with their 12.5" f/5 Home made Newtonian and SBIG ST8i NAGB CCD camera with enhanced cooling. This is an LRGB composite image, exposed LRGB = 80:20:20:40.

  • More information on this image (C. & D. Schur)

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    References:


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