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Caldwell 5 — Galaxy in Camelopardalis

IC 342

Galaxy Excellent (70/100)

Barred Spiral

Magnitude 9.2m Galaxy Camelopardalis Visible
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About C5

Description

IC 342 is a face-on spiral galaxy in Camelopardalis, about 10.7 million light-years away. It would be one of the brightest galaxies in the sky if not heavily obscured by dust in our Milky Way's disk. It is the principal member of the IC 342/Maffei group.

Observing Tips

A challenging target due to heavy Milky Way foreground extinction. Requires dark skies and at least a 6-inch telescope. Appears as a large, very faint, diffuse glow. Use low power and averted vision. Best on autumn and winter evenings.

History

Discovered by W.F. Denning in 1892. Its proximity was not recognized until later because foreground extinction dims it by several magnitudes. Sometimes called the "Hidden Galaxy."

Fun Facts

If IC 342 were not behind the Milky Way's dust, it would be visible to the naked eye and rival M31 in apparent brightness. It has an active nucleus and vigorous star formation in its spiral arms.

Observe

1Properties

Magnitude 9.2
Angular Size 19.8′ × 18.8′
Position Angle
Distance 10.50 million ly
Galaxy Type Barred Spiral (SABc)
Spiral Galaxy [Distance: 10500000 ly]

Position & Identifiers

RA 03h 46m 48.0s
Dec +68° 05' 60.0"
Constellation Camelopardalis
Catalog C5
Also known as IC 342

2How easy to spot?

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Telescope Bortle 3 Bortle 4 Bortle 5
80mm refr. V. hard+ V. hard Imp.
150mm Newt. Hard+ Hard Hard
C8 203mm Hard+ Hard+ Hard
Easy Medium Hard Very hard Impossible

Bortle 3 = rural · 4 = outer suburbs · 5 = suburbs

Easy on Seestar S50

3Visibility

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Best season Oct – Dec (peak: Nov)

4 Eyepiece View

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50x TFOV: 1.0° Lim. mag: 13.6
N E

C5 · 19.8′×18.8′ · N up, E left

5 Best Magnification

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6 Surface Brightness

7 Morphology Decoder

8 Inclination & True Shape

9 Redshift

10 Size Comparator

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Light Travel Time Machine

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Relativistic Travel

Community Photos (1)

Credit: ESA/Euclid/Euclid Consortium/NASA image processing by J.-C. Cuillandre (CEA Paris-Saclay) G. Anselmi. License: CC BY-SA 3.0 igo. (Wikimedia Commons)

Credit: ESA/Euclid/Euclid Consortium/NASA image processing by J.-C. Cuillandre (CEA Paris-Saclay) G. Anselmi. License: CC BY-SA 3.0 igo. (Wikimedia Commons)

Skybred Mar 2, 2026

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