M13 is a spectacular globular cluster and the best example of its type in the northern section of the sky. It's the standout deep sky object in the constellation of Hercules and is sometimes referred to as the Great Hercules Globular Cluster. At mag. +5.8, M13 is just about visible to the naked eye and an easy binocular target. The popularity of M13 is mainly due to its declination; it lies at 36 degrees north and is therefore well placed and appears high in the sky during the summer months from northern temperate latitudes. There are many other globulars larger and brighter than M13, but all are located in the southern section of the sky. As a result, they either never rise or always appear low down from North America, European and Asian locations. Hence, M13 is perhaps the most observed and studied globular cluster of all.

M13 was discovered by the Astronomer Royal, Sir Edmond Halley in 1714. He described it as "a little patch, but shews itself to the naked eye, when the sky is serene and the Moon is absent". Fifty years later, Charles Messier catalogued it on June 1, 1764.

M13 Globular Cluster (credit:- NASA, ESA, and The Hubble Heritage Team (STScI/AURA))

Finder Chart for M13 (credit:- freestarcharts)

Finder Chart for M13 - pdf format (credit:- freestarcharts)

The globular is easily found on the western side of the Hercules "Keystone" asterism, 2.5 degrees south of Eta Herculis (η Her) and along a line connecting Eta Herculis (η Her) with Zeta Herculis (ζ Her). When viewed through 10x50 binoculars, it appears as bright fuzzy ball with a well-defined center that's obviously non-stellar but without resolution. The cluster forms a right angled triangle with two nearby 7th magnitude stars. An 80 mm (3.1-inch) telescope shows M13 as a uniform extended hazy disk about 8 arc minutes across. At magnifications of about 100x, it appears like a zoomed in version of the binocular view. A 100mm (4-inch) telescope will resolve some of the outer stars, with many more visible in 150mm (6-inch) and 200mm (8-inch) instruments. The brightest star in M13 is variable star V11 (apparent mag. +11.95).

In large amateur telescopes, M13 is truly sensational sight with the complete field awash with stars. When viewed through a 250mm (10-inch) scope, hundreds of stars are visible against the dark background sky. The cluster appears 3-dimensional and breathtaking. In total, it has an apparent size of about 20 arc minutes, though visually it appears smaller, perhaps 12-13 arc minutes across. There are a couple of curious affects visible at a high magnification. Many of the outer stars seem to be arranged in long arcs, weaving their way across the cluster face and the distribution of the bright stars across the surface is not even. This can result in an optical illusion of apparent voids or relatively barren areas interspersed across the cluster. Also visible at medium/high magnifications in telescopes of the order of 300mm (12-inch) are three dark dust lanes that form a Y shape towards the southeast of the core. This is known as the "propeller" and was first noticed by Bindon Stoney in the 1850s from Birr Castle in Ireland using the 72-inch reflector, the largest telescope in the World at the time.

The globular is located 25,100 light-years from Earth. It has a spatial diameter of 145 light-years and is estimated to contain about 300,000 stars. M13 appears big and bright due to its close proximity, not because it's intrinsically luminous or large. In 1974, M13 was chosen as the target for the Arecibo radio message. This was designed to communicate the existence of human life to hypothetical extraterrestrials that may live on a planet orbiting one of the thousands of stars in M13. The test was more of a technological demonstration than a realistic communications effort. Since the signal will take 25,100 years to arrive, M13 will have moved position and no longer be in the correct location to receive it.

M13 Data Table

Messier13
NGC6205
NameGreat Hercules Globular Cluster
Object TypeGlobular Cluster
ConstellationHercules
Distance (kly)25.1
Apparent Mag.5.8
RA (J2000)16h 41m 41s
DEC (J2000)36d 27m 41s
Apparent Size (arc mins)20 x 20
Radius (light-years)72.5
Age (years)11,650M
Number of Stars300,000

Sky Highlights - January 2017

Conjunction
Mars passes just 1 arc minute south of Neptune on January 1, 2017

Comet
Comet 45P/Honda-Mrkos-Pajdusakova now visible with small telescopes

Meteor Shower
Quadrantids meteor shower peaks on January 3, 2017

Minor Planet
Vesta now visible with binoculars and small telescopes. Reaches opposition on January 17, 2017

The Planets
This Month's Guide

Algol Minima
Algol eclipse dates and times for January 2017

Northern Hemisphere
Evening
Southwest:- Venus (mag. -4.4 to -4.7), Mars (mag. +0.9 to +1.1), Neptune (mag. +8.0)
South:- Uranus (mag. +5.8)
Midnight
West:- Uranus
East:- Jupiter (mag. -1.9 to -2.1)
Morning
South:- Jupiter (mag. -1.8)
Southeast:- Saturn (mag. +0.6), Mercury (mag. -0.2 second half of month)

Southern Hemisphere
Evening
West:- Venus, Mars, Neptune
Northwest:- Uranus
Midnight
East:- Jupiter
Morning
Northeast:- Jupiter
East:- Saturn, Mercury (second half of month)

Deep Sky
Naked eye / binoculars:-
Messier 45 - M45 - The Pleiades (Open Cluster)
The Hyades - Open Cluster
NGC 869 and NGC 884 - The Double Cluster - Open Clusters
Messier 31 - M31 - Andromeda Galaxy (Spiral Galaxy)
Messier 42 - M42 - The Great Orion Nebula (Emission/Reflection)

Small telescopes:-
NGC 457 - Owl Cluster - Open Cluster
Messier 103 - M103 - Open Cluster
Messier 36 - M36 - Open Cluster
Messier 37 - M37 - Open Cluster
Messier 38 – M38 - Open Cluster

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