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NGC 2298

NGC 2298 is a globular cluster in Puppis.

It was discovered by James Dunlop on May 30, 1826, and is likely a former member of the disputed Canis Major Dwarf galaxy.

Apparent mag.9.3
Surface brightness13.2
Size6.8 ‘
Class6
StarsBrightest star: 13.4m
Dreyer’s description GC B pL iR gbM rr

NGC 2298 has been observed with the following:

  • Telescopes up to 70mm
  • Telescopes 71mm – 100mm (2.8″ – 3.9″)
  • Telescopes 101mm – 141mm (4″ – 5.5″)
  • Telescopes 141mm – 177mm (5.6″ – 6.9″)
  • Telescopes 178mm – 234mm (7″ – 9.2″)
  • Telescopes 235mm – 305mm (9.25″ – 12″)
  • Telescopes 306mm – 381mm (12.1″ – 15″)
  • Telescopes above 15″
  • Binoculars up to 50 mm, and finders
  • Binoculars 51mm – 70mm
  • Binoculars 71mm – 100mm

If you are looking to observe this cluster, for telescopes I recommend either the Celestron Nexstar 6se, or 8se.

For binoculars, I recommend the Celestron SkyMaster 20×80 or 25×100.