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Caldwell 58 — Open Cluster in Canis Major

NGC 2360

Open Cluster Excellent (70/100)
Magnitude 7.2m OpenCluster Canis Major Visible
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About C58

Description

NGC 2360 is an open cluster in Canis Major, about 3,700 light-years away. It is a rich, well-concentrated cluster containing about 80 stars within 13 arcminutes, with an age of roughly 2.2 billion years.

Observing Tips

A fine cluster in a 4-inch telescope at medium power. The background Milky Way star field adds to the view. Many of the cluster stars are similar in brightness, giving it an even, grainy appearance. Best in winter evenings.

History

Discovered by Caroline Herschel on February 26, 1783. It is one of the notable discoveries by William Herschel's sister, a pioneering astronomer in her own right.

Fun Facts

Caroline Herschel discovered this cluster using a small refractor while conducting her own independent sky surveys. She discovered 8 comets and several nebulae and clusters during her career.

Observe

1Properties

Magnitude 7.2
Angular Size 9.0′
Distance 3,700 ly
Open Cluster [Distance: 3700 ly]

Position & Identifiers

RA 07h 17m 43.2s
Dec -15° 38' 27.6"
Constellation Canis Major
Catalog C58
Also known as NGC 2360
Physical size
9.6 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 180 of 677 members.

3Visibility

Set a location in User Settings to see visibility data.

Best season Dec – Feb (peak: Jan)

4 Eyepiece View

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125x TFOV: 0.4° Lim. mag: 13.6
N E

C58 · 9.0′ 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 C58 1.0 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

Discover

9

Light Travel Time Machine

10

Relativistic Travel

Community Photos (1)

Credit: Sloan Digital Sky Survey. License: CC BY 4.0. (Wikimedia Commons)

Credit: Sloan Digital Sky Survey. License: CC BY 4.0. (Wikimedia Commons)

Skybred Mar 2, 2026

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