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Caldwell 96 — Open Cluster in Carina

NGC 2516

Open Cluster Showpiece (91/100)
Magnitude 3.8m OpenCluster Carina Visible
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About C96

Description

NGC 2516 is a large, bright open cluster in Carina, about 1,300 light-years away. At magnitude 3.8 it is easily visible to the naked eye, spanning 30 arcminutes and containing over 100 stars. It is sometimes called the Southern Beehive due to its resemblance to M44.

Observing Tips

An excellent naked-eye and binocular cluster. Too large for most telescopes at high power — binoculars or a wide-field scope at low power give the best view. Several red giants provide color contrast. Best from southern latitudes in late winter and spring.

History

Discovered by Nicolas Louis de Lacaille in 1751. It is one of the brightest clusters visible from southern latitudes and a standard comparison to the northern Beehive Cluster (M44).

Fun Facts

NGC 2516 is about 140 million years old, similar to the Pleiades. X-ray observations have detected many magnetically active stars, and the cluster has been used to study the rotation rates and activity levels of solar-type stars.

Observe

1Properties

Magnitude 3.8
Angular Size 24.3′
Distance 1,300 ly
Open Cluster [Distance: 1300 ly]

Position & Identifiers

RA 07h 58m 03.6s
Dec -60° 52' 01.2"
Constellation Carina
Catalog C96
Also known as NGC 2516
Physical size
9.8 light-years across — about 2.2× the Sun-to-Alpha-Centauri distance

2How easy to spot?

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Telescope Bortle 3 Bortle 4 Bortle 5
80mm refr. Easy Easy Easy
150mm Newt. Easy Easy Easy
C8 203mm Easy Easy Easy
Easy Medium Hard Very hard Impossible

Bortle 3 = rural · 4 = outer suburbs · 5 = suburbs

Easy on Seestar S50
At 150mm under B5 skies you should resolve about 232 of 650 members.

3Visibility

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Best season Dec – Feb (peak: Jan)

4 Eyepiece View

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50x TFOV: 1.0° Lim. mag: 13.6
N E

C96 · 24.3′ diameter

5 Best Magnification

6Where this cluster sits in time

1 Myr 10 Myr 100 Myr 1 Gyr 10 Gyr NGC 2362 Hyades M67 NGC 188 C96 240 Myr

Open clusters span more than four orders of magnitude in age — from newborn OB associations to ancient, metal-rich survivors.

7 Colour-Magnitude Diagram

A cluster's colour-magnitude diagram reveals its age: the bluer the turn-off point where the main sequence bends into red giants, the younger the cluster.

Loading member data…

Each point is a Gaia-DR3 member. Colour encodes spectral type; size reflects membership probability.

Explore

8 Classification Decoder

Discover

9

Light Travel Time Machine

10

Relativistic Travel

Community Photos (1)

Credit: G Furtado. License: CC BY-SA 4.0. (Wikimedia Commons)

Credit: G Furtado. License: CC BY-SA 4.0. (Wikimedia Commons)

Skybred Mar 2, 2026

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