NGC 4945
Properties
Position & Identifiers
Visibility
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Eyepiece View
NGC 4945 · 23.3′×4.0′ · N up, E left
Surface Brightness & Visibility
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About NGC 4945
Description
NGC 4945 is a bright, edge-on barred spiral galaxy in Centaurus, about 11.7 million light-years away. It is one of the brightest galaxies in the Centaurus A/M83 galaxy group and hosts a Seyfert 2 active nucleus obscured by heavy dust absorption.
Observing Tips
Visible as a bright, elongated streak in a 6-inch telescope. The thick dust lane makes the profile appear asymmetric. Located near Centaurus A (C77). Best from southern latitudes in spring and summer evenings.
History
Discovered by James Dunlop on April 30, 1826 from Australia. X-ray and infrared observations have revealed the hidden active galactic nucleus behind the galaxy's dust-choked central region.
Fun Facts
NGC 4945's central supermassive black hole is accreting matter and producing powerful water maser emission — one of the strongest extragalactic maser sources known, visible at radio wavelengths.