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Caldwell 85 — Open Cluster in Vela

IC 2391

Open Cluster Showpiece (95/100)
Magnitude 2.5m OpenCluster Vela Visible
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About Omicron Velorum Cluster

Description

The Omicron Velorum Cluster (IC 2391) is a bright, nearby open cluster in Vela, about 574 light-years away. At magnitude 2.5, it is easily visible to the naked eye and contains about 30 stars spanning 50 arcminutes, centered on the bright star Omicron Velorum.

Observing Tips

A fine naked-eye and binocular cluster. Too spread out for most telescopes — binoculars at 7-10x give the best view. The cluster is dominated by Omicron Velorum (mag 3.6). Best from southern latitudes in late winter and spring.

History

Known since antiquity as a naked-eye grouping. First cataloged by Nicolas Louis de Lacaille in 1751. It was one of the clusters used to determine the age of nearby stellar associations.

Fun Facts

At only 50 million years old, IC 2391 is a young cluster whose stars are still settling down. Several of its stars show strong X-ray emission characteristic of magnetically active young stars.

Observe

1Properties

Magnitude 2.5
Angular Size 29.1′
Distance 574 ly
Open Cluster [Distance: 574 ly]

Position & Identifiers

RA 08h 40m 16.6s
Dec -53° 03' 32.4"
Constellation Vela
Catalog C85
Also known as IC 2391
Physical size
4.1 light-years across — about 0.9× 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 63 of 222 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

Omicron Velorum Cluster · 29.1′ diameter

5 Best Magnification

6Where this cluster sits in time

1 Myr 10 Myr 100 Myr 1 Gyr 10 Gyr NGC 2362 Pleiades Hyades M67 NGC 188 Omicron Velorum Cluster 29 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: YayLol123. License: CC BY-SA 4.0. (Wikimedia Commons)

Credit: YayLol123. License: CC BY-SA 4.0. (Wikimedia Commons)

Skybred Mar 2, 2026

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