NGC 6846 (Lund 912, Cr 410) Open Cluster in Cygnus
Located at: RA 19 hours 56 minutes 28 seconds, Dec +32 degrees 20 minutes 55 seconds
Size: 0.8'; Magnitude: 14.2v; Class: II 2 -- (IV 1 p)*
North is up

West to the right
| Telescope: |
8" f5 Newtonian reflector |
| Camera: |
ST-8XME, self-guided, binned 1x1, temp -15c, camera control MaxIm DL 4.56 |
| Image: |
Lumicon Deep Sky filter, 300 minutes (30 x 10 minute subs), 08/2/3/2007 |
| Processing: |
CCDStack 1.2, Photoshop 7.0 |
| Location: |
Rolling Roof Observatory, Thousand Oaks, CA 91360 (+34d 13m 29s -118h 52m 20s) |
| Notes:* | According to "Star Clusters", by Brent Archinal
and Steven Hynes, this little open cluster has had a positional error of 2 degrees too
far South in most references published since 1931 (by Collinder ...
Collinder
410). From the NGC / IC Project: Contemporary Visual Observation(s) for NGC 6846NGC 6846 = Lund 912 = OCL-139 = Cr 410 19 56 28.1 +32 20 58 V = 14.2; Size 0.8 17.5": at 225x appears as a small, faint clump of stars over unresolved haze. Elongated about 3:2 E-W with dimensions 1.5'x1.0'. A mag 13.5 star is off the NW edge, a mag 14 star is at the W edge and three additional mag 14 stars in a clump are just visible over of the haze although clean resolution is difficult. The extremely faint stellar planetary K4-41 is 2' NE! The position given in RNGC, Lynga, N2000 and U2000 is exactly two degrees too far south. Discovered by Stephan and correctly placed at 19 56 28.7 +32 21 16 (2000). RNGC lists this open cluster at 19h 56.5m +30 21 (2000) or two degrees south of Stephan's position and I unsuccessfully searched for the cluster at this position with my 17.5" scope. The incorrect position in the RNGC is also found in the Lynga #5 catalogue (source of the orignal error?) and is repeated in NGC 2000, DSFG and on the U2000 star atlas. Listed in RNGC Corrections #6. See Corwin's NGCBUGS. - by Steve GottliebHistorical Research Notes / Correction for NGC 6846 NGC 6846. The RNGC position is 2 degrees too far south. At the correct position is a compact little cluster matching Stephan's description exactly: the three brightest stars are clear enough that he could see them, but the others are considerably fainter, so the entire group must have looked quite nebulous to him. - Dr. Harold G. Corwin, Jr. There is a very small (3") Planetary Nebula (PK68+1.1) about 1.9 minutes NNE of this cluster (looks like a small star at this focal length) |