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Caldwell 14 — Open Cluster in Perseus

NGC 869

Open Cluster Showpiece (77/100)
Magnitude 4.3m OpenCluster Perseus Visible
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About Double Cluster

Description

The Double Cluster (NGC 869 and NGC 884) is a pair of open clusters in Perseus, about 7,500 light-years away. Together they span about 60 arcminutes and contain several hundred stars each, including many blue supergiants. At magnitude 4.3, the pair is visible to the naked eye.

Observing Tips

A showpiece object, stunning in binoculars and small telescopes at low power (25-40x). Each cluster fills about half a degree, so a wide field of view is ideal. Look for colorful orange and red supergiants scattered among the blue-white stars. Best in autumn and winter.

History

Known since antiquity; Hipparchus noted a bright patch between Perseus and Cassiopeia around 130 BC. Messier inexplicably left it out of his catalog, which is one reason Patrick Moore created the Caldwell catalog.

Fun Facts

The two clusters are physically related and only a few hundred light-years apart in space. At just 12-14 million years old, they are among the youngest known clusters. If our Sun were located in the Double Cluster, the night sky would contain hundreds of stars brighter than Sirius.

Observe

1Properties

Magnitude 4.3
Angular Size 14.4′
Distance 7,300 ly
Open Cluster [Distance: 7300 ly]

Position & Identifiers

RA 02h 20m 42.0s
Dec +57° 07' 58.8"
Constellation Perseus
Catalog C14
Also known as NGC 869
Physical size
30 light-years across — about 3.5× 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 128 of 501 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

Double Cluster · 14.4′ 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 Double Cluster 15 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: Genuson. License: CC BY-SA 3.0. (Wikimedia Commons)

Credit: Genuson. License: CC BY-SA 3.0. (Wikimedia Commons)

Skybred Mar 2, 2026

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