M107 is a loose eight-magnitude globular cluster located in Ophiuchus that's a difficult binocular object but much easier in small telescopes. It was discovered by Pierre Méchain in April, 1782 and then independently re-discovered by William Herschel on May 12, 1793. Herschel was also the first person to resolve M107 into stars. This cluster is one of the additional catalogue items that weren't included in Messier's final version but added much later by Helen Sawyer Hogg in 1947. She also added M105 and M106 since it seems probable that Méchain had also intended to include these items to a future edition of the catalogue.

The globular is located 20,900 light-years from Earth and spans 13 arc minutes of apparent sky, which corresponds to a spatial diameter of 80 light-years. It contains 100,000 stars and has an estimated age of 13.95 billion years, making it one of the oldest known globulars.

Locating M107 is relatively easy as its positioned 2.75 degrees southwest of zeta Oph (ζ Oph - mag. +2.5). This star is located 16 degrees north of Antares (α Sco - mag. +1.0) and can be also found by imagining a line connecting Yed Prior (δ Oph - mag. +2.7) with Yed Posterior (ε Oph - mag. +3.2) and extending it in a south-easterly direction for 9 degrees. The cluster is best observed during the months of May, June and July.

M107 globular cluster by the Hubble Space Telescope (NASA, The Hubble Heritage Team (AURA/STScI))

Finder Chart for M107 (also shown M4, M9, M19 and M80)

Finder Chart for M107 (also shown M4, M9, M19 and M80) - pdf format

Finder Chart for M9 (also shown M4, M8, M19->M21, M23, M80 and M107)

Finder Chart for M9 (also shown M4, M8, M19->M21, M23, M80 and M107) - pdf format

At magnitude +8.0, M107 appears as a faint small diffuse object through a small 80mm (3.1-inch) telescope. There is a subtle increase in brightness from the outer to the inner region but no particularly bright centre. A 150mm (6-inch) scope will start to show the brighter stars around the outer edges but the view is much better with larger telescopes. Instruments of 300mm (12-inch) aperture or greater reveal an incredible site, many stars visible across the entire face of the globular. What's also noticeable is the looseness of this cluster.

At least 25 known variable stars have been identified in M107. It seems to contain some regions obscured by darkness, which is unusual for globular clusters.

M107 Data Table

Object TypeGlobular cluster
Distance (kly)20.9
Apparent Mag.8.0
RA (J2000)16h 32m 32s
DEC (J2000)-13d 03m 10s
Apparent Size (arc mins)13 x 13
Radius (light-years)40
Age (years)13,950M
Number of Stars100,000

Sky Highlights - March 2017

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

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
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)
Southeast:- Jupiter (mag. -2.3 to -2.5)
Southwest:- Jupiter
Southeast:- Saturn (mag. +0.5)

Southern Hemisphere
West:- Venus (first half of month), Mars, Uranus
North:- Jupiter
East:- Saturn
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)

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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