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The Perseus–Pisces Supercluster is one of two dominant concentrations of galaxies (the other being the Local supercluster) in the nearby universe (within 300 million light years). This supercluster also borders a prominent void, the Taurus Void, and is part of the Perseus–Pegasus Filament which stretches for roughly a billion light years. [1]
NGC 1259 is a lenticular galaxy [2] located about 243 million light-years away [3] in the constellation Perseus. [4] The galaxy was discovered by astronomer Guillaume Bigourdan on October 21, 1884 [5] and is a member of the Perseus Cluster. [6] [5] A type Ia supernova designated as SN 2008L was discovered in NGC 1259 on January 14, 2008. [7] [8 ...
Perseus Cluster (24 P) Pages in category "Perseus-Pisces Supercluster" The following 7 pages are in this category, out of 7 total.
IC 348 south of Omicron Persei. IC 348 is a star-forming region in the constellation Perseus located about 1,000 light years from the Sun. It consists of nebulosity and an associated 2-million-year-old cluster of roughly 400 stars within an angular diameter of 20″.
UGC 2885 (Rubin's Galaxy, [10] nicknamed "Godzilla galaxy" [11]) is a large barred spiral galaxy of type SA(rs)c in the constellation Perseus.It is 232 million light-years (71 Mpc) from Earth and measures 463,000 ly (142,000 pc) across, making it one of the largest known spiral galaxies.
NGC 1283 is an elliptical galaxy [2] located about 250 million light-years away [3] in the constellation Perseus. [4] The galaxy was discovered by astronomer Guillaume Bigourdan on October 23, 1884 [5] and is a member of the Perseus Cluster. [6] [5] It also contains an active galactic nucleus. [7]