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Caldwell 13 — Open Cluster in Cassiopeia

NGC 457

Open Cluster Excellent (70/100)
Magnitude 6.4m OpenCluster Cassiopeia Visible
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About Owl Cluster

Description

The Owl Cluster (NGC 457) is a bright open cluster in Cassiopeia, about 7,900 light-years away. It features two bright stars that form the "eyes" of an owl with wings spread, giving it its popular name. The cluster spans about 13 arcminutes.

Observing Tips

One of the most delightful open clusters for beginners. Even a small telescope reveals the owl pattern clearly. The bright star Phi Cassiopeiae marks one eye. Best at 40-60x to frame the entire figure. Circumpolar and best in autumn.

History

Discovered by William Herschel in 1787. Also known as the E.T. Cluster because some observers see the outline of the movie character E.T. instead of an owl.

Fun Facts

Whether Phi Cassiopeiae (the bright yellow star forming one eye) is actually a cluster member or a foreground star is debated. If it is a member, it would be one of the most luminous supergiants known.

Observe

1Properties

Magnitude 6.4
Angular Size 7.8′
Distance 7,900 ly
Open Cluster [Distance: 7900 ly]

Position & Identifiers

RA 01h 19m 30.0s
Dec +58° 19' 58.8"
Constellation Cassiopeia
Catalog C13
Also known as NGC 457
Physical size
20 light-years across — about 2.4× 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 88 of 508 members.

3Visibility

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Best season Sep – Nov (peak: Oct)

4 Eyepiece View

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125x TFOV: 0.4° Lim. mag: 13.6
N E

Owl Cluster · 7.8′ 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 Owl Cluster 21 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.

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8 Classification Decoder

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9

Light Travel Time Machine

10

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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