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NGC 208

Spiral galaxy in the constellation Pisces

Wikipedia contributorsAdapted for Fathomly · View authors
1 min read
Source updated September 3, 2026
Image credit is listed at the end of this article.

NGC 208 is a spiral galaxy located approximately 229 million light-years from the Solar System in the constellation Pisces. It was discovered on October 5, 1863, by Albert Marth.

01Supernova

One supernova has been observed in NGC 208: SN 2024luo (type Ia, mag. 17.2).

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Sources and credits

This article is adapted from the Wikipedia article “NGC 208”, written by its contributors and licensed under CC BY-SA 4.0. Fathomly has changed the layout, removed citation markers, navigation and maintenance notices, and adjusted punctuation. This adapted version is shared under the same license. For references, see the original article.

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Related topics

Spiral galaxy

Spiral galaxies form a class of galaxy originally described by Edwin Hubble in his 1936 work The Realm of the Nebulae and, as such, form part of the Hubble sequence. Most spiral galaxies consist of a flat, rotating disk containing stars, gas and dust, and a central concentration of stars known as the bulge.

List of NGC objects (1-1000)

This is a list of NGC objects 1-1000 from the New General Catalogue. The astronomical catalogue is composed mainly of star clusters, nebulae, and galaxies.

Pisces (constellation)

Pisces is a constellation of the zodiac. Its vast bulk, and main asterism viewed in most European cultures per Greco-Roman antiquity as a distant pair of fishes connected by one cord each that join at an apex, are in the Northern celestial hemisphere.