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Caldwell 71 — Open Cluster in Puppis

NGC 2477

Open Cluster Showpiece (82/100)
Magnitude 5.8m OpenCluster Puppis Visible
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About C71

Description

NGC 2477 is one of the richest open clusters in the sky, located in Puppis about 3,600 light-years away. It contains roughly 300 stars within a diameter of 27 arcminutes and has sometimes been mistaken for a globular cluster due to its dense concentration.

Observing Tips

A spectacular cluster in any telescope. Binoculars show a rich, hazy patch. A 4-inch telescope resolves dozens of stars, and an 8-inch scope at 80-120x is breathtaking with hundreds of stars filling the field. Best in winter evenings.

History

Discovered by Nicolas Louis de Lacaille in 1751 from South Africa during his southern sky survey. It is considered one of the finest open clusters in the southern sky.

Fun Facts

NGC 2477 is about 700 million years old and so rich that its total mass and density approach those of a sparse globular cluster. It is one of the most massive open clusters in the Milky Way.

Observe

1Properties

Magnitude 5.8
Angular Size 18.6′
Distance 3,700 ly
Open Cluster [Distance: 3700 ly]

Position & Identifiers

RA 07h 52m 12.2s
Dec -38° 31' 58.8"
Constellation Puppis
Catalog C71
Also known as NGC 2477
Physical size
25 light-years across — about 3.0× the Sun-to-Sirius 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 241 of 800 members.

3Visibility

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Best season Dec – Feb (peak: Jan)

4 Eyepiece View

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125x TFOV: 0.4° Lim. mag: 13.6
N E

C71 · 18.6′ diameter

5 Best Magnification

6Where this cluster sits in time

1 Myr 10 Myr 100 Myr 1 Gyr 10 Gyr NGC 2362 Pleiades M67 NGC 188 C71 1.1 Gyr

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

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9

Light Travel Time Machine

10

Relativistic Travel

Community Photos (1)

Credit: Guillermo Abramson. License: CC BY 3.0. (Wikimedia Commons)

Credit: Guillermo Abramson. License: CC BY 3.0. (Wikimedia Commons)

Skybred Mar 2, 2026

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