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Caldwell 64 — Open Cluster in Canis Major

NGC 2362

Open Cluster Excellent (71/100)
Magnitude 4.1m OpenCluster Canis Major Visible
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About C64

Description

NGC 2362 is a compact, young open cluster in Canis Major, about 4,800 light-years away. It is dominated by the brilliant magnitude 4.4 blue supergiant Tau Canis Majoris at its center, surrounded by about 60 fainter members within 8 arcminutes.

Observing Tips

A striking sight in small telescopes, with the dazzling Tau CMa surrounded by a spray of fainter stars. Best at 60-100x. The cluster is easy to find as Tau CMa is visible to the naked eye. Best in winter evenings.

History

Discovered by Giovanni Battista Hodierna before 1654. The cluster is only about 5 million years old, making it one of the youngest open clusters known.

Fun Facts

Tau Canis Majoris, the cluster's brightest star, is actually a multiple star system with at least 5 components. The primary is an O-type supergiant about 50,000 times more luminous than the Sun and will likely explode as a supernova.

Observe

1Properties

Magnitude 4.1
Angular Size 7.2′
Distance 5,100 ly
Open Cluster [Distance: 5100 ly]

Position & Identifiers

RA 07h 18m 41.5s
Dec -24° 57' 14.4"
Constellation Canis Major
Catalog C64
Also known as NGC 2362
Physical size
9.2 light-years across — about 2.1× 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 48 of 144 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

C64 · 7.2′ diameter

5 Best Magnification

6Where this cluster sits in time

1 Myr 10 Myr 100 Myr 1 Gyr 10 Gyr Pleiades Hyades M67 NGC 188 C64 5.8 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.

Discover

8

Light Travel Time Machine

9

Relativistic Travel

Community Photos (1)

Credit: Chuck Ayoub. License: CC0. (Wikimedia Commons)

Credit: Chuck Ayoub. License: CC0. (Wikimedia Commons)

Skybred Mar 2, 2026

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