M92
From South Dublin Astronomical Society
| M92 | |
|---|---|
| Type | Globular cluster |
| NGC | NGC 6341 |
| Constellation | Hercules |
| Right Ascension | 17h 17.1m |
| Declination | +43° 08' |
| Magnitude | 6.5 |
| Size | 11 arc min. |
| | |
| Image:M92 messier image.jpg | |
Hercules hosts another Messier globular, M92, which languishes somewhat
in observing backwaters because of it’s proximity to the more illustrious
M13. It’s a little more distant too than M13 at 26,700 light-years and
looks more condensed in binoculars – you might confuse it with a similarly
bright star a little to the east if your instruments are not perfectly focussed.
There’s a lovely scattering of many faint stars below the cluster in the
same field that vague trace out a large southwest pointing arrowhead. To
find M92, scan a little over one 5° binocular field-width north from Pi (π)
Herculis, the star marking the top-left corner of the “Keystone” asterism.
A piece of trivia is that the effect of precession of the Earth’s axis over
a 25,800 year period causes the North Celestial Pole to pass within one
degree of the cluster. Such was the case about 10,000 BC and this will next
occur in 16,000 AD. A case of multiple (but very faint) Pole Star’s perhaps?
M1 | M2 | M3 | M4 | M5 | M6 | M7 | M8 | M9 | M10 | M11 | M12 | M13 | M14 | M15 | M16 | M17 | M18 | M19 | M20 | M21 | M22 | M23 | M24 | M25 | M26 | M27 | M28 | M29 | M30 | M31 | M32 | M33 | M34 | M35 | M36 | M37 | M38 | M39 | M40 | M41 | M42 | M43 | M44 | M45 | M46 | M47 | M48 | M49 | M50 | M51 | M52 | M53 | M54 | M55 | M56 | M57 | M58 | M59 | M60 | M61 | M62 | M63 | M64 | M65 | M66 | M67 | M68 | M69 | M70 | M71 | M72 | M73 | M74 | M75 | M76 | M77 | M78 | M79 | M80 | M81 | M82 | M83 | M84 | M85 | M86 | M87 | M88 | M89 | M90 | M91 | M92 | M93 | M94 | M95 | M96 | M97 | M98 | M99 | M100 | M101 | M102 | M103 | M104 | M105 | M106 | M107 | M108 | M109 | M110