M 72 (NGC 6981) Globular Cluster in Aquarius
Located at: RA 20 hours 53 minutes 28 seconds, Dec -12 degrees 32 minutes 13 seconds
Size: 6.6'; Magnitude: 9.2; Class: 9
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, 240 minutes (24 x 10 minute subs), 10/8/9/2007 |
| Processing: |
CCDStack 1.3, Photoshop 7.0 |
| Location: |
Rolling Roof Observatory, Thousand Oaks, CA 91360 (+34d 13m 29s -118h 52m 20s) |
| Notes: |
From the NGC / IC Project: Contemporary Visual Observation(s) for NGC 6981 NGC 6981 = M72 20 53 27.9 -12 32 13 V = 9.2; Size 6 17.5" (7/17/01): at 380x, the halo is very irregular and the globular has a very uneven surface brightness. The non-symmetrical halo is elongated ~E-W, perhaps 4'x3'. The brighter 1.5' core is covered with a sprinkling a 8-10 faint stars. From the core there are short ragged extensions to the SW and NW with a few resolved stars. More prominent is a nearly detached clump on the E side which is extended ~N-S and contains roughly 8 easily resolved stars over haze. In total, perhaps two dozen stars are resolved in moments of good seeing. 17.5" (8/13/88 and 8/2/86): very mottled ragged appearance, 3' diameter. About 20 stars are resolved at the edges and over the core. 13" (9/29/84): very mottled non-symmetrical appearance with a bright core. Roughly a dozen stars are resolved mostly on the E side of the core. A brighter mag 13.5 star is in the NE side of the halo. - by Steve Gottlieb |