NGC 1333 (LBN 741) Bright Nebula complex in Perseus
Located at: RA 03 hours 29 minutes 15 seconds, Dec +31 degrees 23 minutes 52 seconds
Size: 4.8' x 2.8'; Magnitude: --; Class: Reflection
North is up

West to the right
| Telescope: |
8" f5 Newtonian reflector |
| Camera: |
ST-8XME, self-guided, binned 1x1, temp -20c & -25c, camera control MaxIm DL 4.56 |
| Image: |
Lumicon Red filter, 820 minutes (82 x 10 minute subs), 11/28/29 & 12/1/2010; seeing 2.8-4.9 FWHM per CCDStack |
| Processing: |
CCDStack 2.16.3986.25838, Photoshop 7.0 |
| Location: |
Rolling Roof Observatory, Thousand Oaks, CA 91360 (+34d 13m 29s -118h 52m 20s) |
| Notes: |
This is a re-shoot of this very complex area of the sky. Unfortunately, the seeing was very poor for two of the three nights I imaged this area; see original 400 minute image ... see Robert Gendler's write up of this area ... and check out his color image. Also see this wider field image of the area from Greg Parker at the Earth Science Picture of the Day site. From the NGC / IC Project: Contemporary Visual Observation(s) for NGC 1333 NGC 1333 = Ced 16 = LBN 741 03 29 19.7 +31 24 57 Size 9x7 17.5" (2/9/02): bright, interesting reflection nebula at 140x. Apparently illuminated by a mag 10 star oddly offset at the NE end of the glow. The appearance is irregular; extending ~10'x6' SW-NE in the general direction of a mag 10 star 11' SW. The SW extension contains a couple of faint mag 14 stars and ends at a small, brighter knot which appears to surround a very faint star or stars. The field is oddly void of faint stars and there is a large starless region to the north (this is dark nebula Barnard 2). 17.5" (12/8/90): fairly bright reflection nebula surrounds a mag 10 star which is offset to the NE side of the nebula. This is a large object, about 10'x6' and elongated SW-NE. There is a bright knot in the SW end. Two or three 15th magnitude stars are superimposed. 13": fairly bright nebula, large, extends SSW of a mag 9.5 star, oval, slightly brighter at the south edge. - by Steve Gottlieb |