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Caldwell 16 — Open Cluster in Lacerta

NGC 7243

Open Cluster Showpiece (81/100)
Magnitude 6.4m OpenCluster Lacerta Visible
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About C16

Description

NGC 7243 is an open cluster in Lacerta, about 2,800 light-years away. It contains around 40 stars spread across 21 arcminutes, with a handful of brighter members at magnitude 8-9 forming distinctive chains and patterns.

Observing Tips

A loose, scattered cluster best seen in binoculars or a wide-field telescope at low power. The brightest stars are easy to resolve. Located in a relatively sparse part of the Milky Way. Best observed in autumn evenings.

History

Discovered by William Herschel in 1788. One of the less famous Herschel discoveries, but a pleasant target for sweeping the autumn Milky Way.

Fun Facts

NGC 7243 is estimated to be about 100 million years old. Its sparse appearance suggests it is gradually dispersing into the general stellar population of the Milky Way.

Observe

1Properties

Magnitude 6.4
Angular Size 15.0′
Distance 2,500 ly
Open Cluster [Distance: 2500 ly]

Position & Identifiers

RA 22h 15m 00.0s
Dec +49° 53' 60.0"
Constellation Lacerta
Catalog C16
Also known as NGC 7243
Physical size
12 light-years across — about 1.5× 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 78 of 289 members.

3Visibility

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Best season Jul – Sep (peak: Aug)

4 Eyepiece View

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125x TFOV: 0.4° Lim. mag: 13.6
N E

C16 · 15.0′ diameter

5 Best Magnification

6Where this cluster sits in time

1 Myr 10 Myr 100 Myr 1 Gyr 10 Gyr NGC 2362 Hyades M67 NGC 188 C16 148 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.

Explore

8 Classification Decoder

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9

Light Travel Time Machine

10

Relativistic Travel

Community Photos (1)

Credit: Egres73. License: CC BY-SA 3.0. (Wikimedia Commons)

Credit: Egres73. License: CC BY-SA 3.0. (Wikimedia Commons)

Skybred Mar 2, 2026

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