NGC 6397 (GC)

Globular Cluster in Ara
R.A.Dec.SizeMag SBCnt.StTypeDistanceChart
17h 40m 43.5s-53° 40′ 20.0″32.0′5.212.4IXGC----
NGC 6397 DSS plate
Source: POSS-2 UK Schmidt Red (STScI) | Field: 48′ × 48′

Background

NGC 6397 is one of the closest globular clusters to the Sun ( 7,800 light-years). Around 13 billion years old — among the very oldest in the Galaxy — and it has undergone “core collapse,” giving it an extremely dense central region. Contains roughly 400,000 stars.

My Observing Notes

25-cm (Meade 10-inch LX200, The Coffee Grinder): Similar size and brightness to M4. The bright core resolves well into lovely chains of stars.(Friday, April 2025)

25-cm (Meade 10-inch LX200, The Coffee Grinder): A perfect way to start the night. Located via the Telrad just below the α/β Ara pair (0.8° apart). Easily picks up the glow in the 9×50 finderscope. At 5.6 mag and 25.7' across, easily resolves into a sea of stars — the dense core gives way to outliers trailing out in loops and arcs, giving it the appearance of a dense open cluster. Filled the FOV in the 26 mm eyepiece.(Friday, June 2025)

References

Charts

NGC 6397 ultra-wide chart
Ultra-wide view (~25° field)
NGC 6397 wide-field chart
Wide-field view with Telrad rings (4°, 2°, 0.5°)
NGC 6397 finderscope view
Finderscope view (9×50 RACI, ~4.4° TFOV)
NGC 6397 eyepiece view
Eyepiece view — 35 mm Panoptic on 12-inch f/5 (1.6° TFOV)