NGC 3766, also known as the Pearl Cluster, is a superb open cluster in Centaurus. At magnitude +5.3, it's faintly visible to the naked eye but challenging to spot against the numerous stars of the background Milky Way. The cluster was born in the Carina molecular cloud, a vast star-forming region that lies at approximately between 6,500 and 10,000 light-years distant. It includes the barely-stable star eta Carinae (η Car), which one-day will explode as a spectacular supernova.

NGC 3766 is a nice binocular target, a wonderful sight through telescopes and one of the jewels of the southern sky. With a declination of 61S, it's best seen from southern latitudes during the months of March, April and May. From many southern towns and cities, the cluster is circumpolar and therefore never sets. However, from northern locations above 29N it never rises above the horizon.

Nicholas Louis de Lacaille discovered NGC 3766 on March 5, 1752.

NGC 3766 (credit:- La Silla Observatory/ESO)

Finder Chart for NGC 3766 (credit:- freestarcharts)

Finder Chart for NGC 3766 - pdf format (credit:- freestarcharts)

The Pearl Cluster is located in the southwestern corner of Centaurus, 7 degrees west and slightly north of Acrux (α Cru - mag. +0.8). Positioned 1.5 degrees south of NGC 3766 is lambda Cen (λ mag. +3.1) and surrounding open cluster and associated emission nebula, IC 2944.

Binoculars show a compact cluster, spanning 12 arc minutes, with a number of stars resolvable. An 80mm (3.1-inch) refractor at 100x magnification reveals a stunning object with dozens of stars visible. Most members are white in colour, but the look is enhanced by a couple of nice 7th magnitude red stars. One red star is positioned left of the cluster centre, the other to the right. The appearance of NGC 3766 has been compared to the Wild Duck Cluster (M11) in Scutum and M37 in Auriga.

Through a medium 200mm (8-inch) scope, NGC 3766 is a stunning sight that appears bright, colourful and fully resolvable. At the extreme northern edge of the cluster lies eclipsing binary BF Cen, which varies between magnitudes +8.5 and +9.4 every 3.7 days. In total, 137 stars have been identified, but it's not clear how many of these are actually members.

NGC 3677 is 5,500 light-years distant and has a spatial diameter of 20 light-years. It's estimated to be 20 million years old.

NGC 3766 Data Table

NamePearl Cluster
Object TypeOpen Cluster
Distance (light-years)5,500
Apparent Mag.+5.3
RA (J2000)11h 36m 14s
DEC (J2000)-61d 36m 36s
Apparent Size (arc mins)12
Radius (light-years)10
Age (years)20 Million
Number of Stars137
Other NamesCollinder 248, Melotte 107

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

Shop at Amazon US

Shop at Amazon US

Current Moon Phase



If you like the website and want to contribute to the running costs then please do so below. All contributions are most welcome.