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Caldwell 1 — Open Cluster in Cepheus

NGC 188

Open Cluster Excellent (61/100)
Magnitude 8.1m OpenCluster Cepheus Visible
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About C1

Description

NGC 188 is one of the oldest known open clusters in our galaxy, estimated at about 6.8 billion years old. Located in Cepheus near the north celestial pole, it lies roughly 5,400 light-years away and contains around 120 stars spread across 14 arcminutes.

Observing Tips

A challenging target requiring at least a 6-inch telescope to resolve individual stars. Located just 4 degrees from Polaris, it is circumpolar from most northern latitudes and can be observed year-round. Best seen at medium power (100-150x).

History

Discovered by John Herschel in 1831. Its extreme age makes it one of the most studied open clusters. Patrick Moore selected it as C1 for his Caldwell catalog, published in 1995 as a complement to the Messier catalog.

Fun Facts

At nearly 7 billion years old, NGC 188 is older than our Sun. Its survival is remarkable because most open clusters are torn apart by gravitational interactions within a billion years. The cluster orbits high above the galactic plane, which may explain how it avoided disruption.

Observe

1Properties

Magnitude 8.1
Angular Size 17.7′
Distance 5,400 ly
Open Cluster [Distance: 5400 ly]

Position & Identifiers

RA 00h 44m 24.0s
Dec +85° 19' 58.8"
Constellation Cepheus
Catalog C1
Also known as NGC 188
Physical size
29 light-years across — about 3.3× 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 35 of 800 members.

3Visibility

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Best season Aug – Oct (peak: Sep)

4 Eyepiece View

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125x TFOV: 0.4° Lim. mag: 13.6
N E

C1 · 17.7′ 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 C1 7.1 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.

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8 Classification Decoder

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9

Light Travel Time Machine

10

Relativistic Travel

Community Photos (1)

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

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

Skybred Mar 2, 2026

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