M15 is one of the brightest and finest globular clusters in the northern section of the sky and the best deep-sky object in the constellation Pegasus. It's only marginally fainter and smaller than M13, the finest northern globular cluster. M15 is relatively easy to find. It's located 4 degrees to the northwest of Enif (ε Peg - mag. +2.4) and at one edge of a right-angled triangle made up of 6th, 7th and 8th magnitude stars.

M15 Globular Cluster (credit:- NASA, ESA, and The Hubble Heritage Team (STScI/AURA))

Finder Chart for M15 (credit:- freestarcharts)

Finder Chart for M15 - pdf format (credit:- freestarcharts)

Finder Chart for M2 (also shown M15) (credit:- freestarcharts)

Finder Chart for M2 (also shown M15) - pdf format (credit:- freestarcharts)

Approaching naked eye visibility under excellent conditions, M15 is easily seen with binoculars or finder scopes appearing as a mag. +6.2 "fuzzy star". A 100mm (4-inch) telescope at low power (40x) reveals a uniformly lit disk, while high powers (>100x) hint at resolution of some of the outer stars. When viewed through a larger 200mm (8-inch) scope, M15 looks like a large bright diffuse ball of light with a dense compact centre. Many stars are resolved in the outer halo, the brightest of which shine at mag. +12.6. Larger instruments do even better. A 300mm (12-inch) scope resolves many stars across the complete disk, creating a spectacular 3-dimensional effect. In total, the globular has an apparent diameter of 18 arc minutes. However, it visually appears somewhat smaller, perhaps only 8 arc minutes across.

M15 is one of the most densely packed globulars known in the Milky Way. Its core has undergone a contraction known as "core collapse" resulting in an enormous number of stars surrounding what may be a central black hole. It's also unusual in that it's one of only four known globulars (along with M22, NGC 6441 and Palomar 6) that contain a planetary nebula. The planetary is named Pease 1.

The cluster was discovered by Italian born French astronomer Jean-Dominique Maraldi on September 7, 1746. It's located 33,600 light-years distant. With an age of at least 12.0 billion years, this is one of the oldest known Milky Way globulars.

M15 Data Table

Messier15
NGC7078
Object TypeGlobular Cluster
ConstellationPegasus
Distance (light-years)33,600
Apparent Mag.+6.2
RA (J2000)21h 29m 58s
DEC (J2000)+12d 10m 00s
Apparent Size (arc mins)18 x 18
Radius (light-years)88
Age (years)12 Billion

Sky Highlights - March 2017

Comet
Comet 41P/Tuttle-Giacobini-Kresak now visible with binoculars as it heads towards perihelion

Mercury
Mercury heading towards greatest elongation east

Minor Planet
Vesta now visible with binoculars and small telescopes.

The Planets
This Month's Guide

Algol Minima
Algol eclipse dates and times for March 2017

Northern Hemisphere
Evening
West:- Venus (mag. -4.8 to -4.1 - first half of month), Mars (mag. +1.3 to +1.5), Uranus (mag. +5.9), Mercury (mag. -1.5 to -0.4 - second half of month)
Midnight
Southeast:- Jupiter (mag. -2.3 to -2.5)
Morning
Southwest:- Jupiter
Southeast:- Saturn (mag. +0.5)

Southern Hemisphere
Evening
West:- Venus (first half of month), Mars, Uranus
Midnight
North:- Jupiter
East:- Saturn
Morning
West:- Jupiter
Northeast:- Saturn
East:- Neptune (mag. +8.0 - second half of month)

Deep Sky
Naked eye / binoculars:-
Melotte 111 - Mel 111 - The Coma Star Cluster (Open Cluster)
Messier 44 - M44 - The Praesepe (Open Cluster)

Telescopes:-
Messier 67 - M67 - Open Cluster
Messier 51 - M51 - The Whirlpool Galaxy (Spiral Galaxy)
Messier 97 - M97 - The Owl Nebula (Planetary Nebula)
Messier 101 - M101 - The Pinwheel Galaxy (Spiral Galaxy)
Messier 65 – M65 – Spiral Galaxy
Messier 66 - M66 - Intermediate Spiral Galaxy
Messier 95 - M95 - Barred Spiral Galaxy
Messier 96 - M96 - Intermediate Spiral Galaxy
NGC 4244 - Spiral Galaxy
NGC 4565 - Needle Galaxy - Spiral Galaxy

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