In today's article, we are going to delve into the exciting world of NGC 684. Whether you're an expert in the field or just starting to explore it, this article has something for everyone. We will explore the most relevant aspects of NGC 684, from its history to its impact on today's society. Additionally, we will discuss the latest trends and discoveries related to NGC 684, as well as opinions from experts in the field. Get ready to embark on a fascinating journey through NGC 684 and discover everything this theme has to offer. Do not miss it!
NGC 684 | |
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![]() NGC 684 (SDSS) | |
Observation data (J2000.0 epoch) | |
Constellation | Triangulum |
Right ascension | 01h 50m 14.0407s [1] |
Declination | +27° 38′ 44.472″ [1] |
Redshift | 0.011798 [1] |
Heliocentric radial velocity | 3537 ± 1 km/s [1] |
Distance | 135.03 ± 3.13 Mly (41.400 ± 0.960 Mpc)[1] |
Group or cluster | NGC 684 group (LGG 32) |
Apparent magnitude (V) | 12.50 [2] |
Apparent magnitude (B) | 13.30 [2] |
Characteristics | |
Type | Sb edge-on [1] |
Size | ~137,500 ly (42.15 kpc) (estimated)[1] |
Apparent size (V) | 3.2′ × 0.6′[1] |
Other designations | |
IRAS 01474+2724, IC 165, UGC 1292, MCG +04-05-017, PGC 6759, CGCG 482-022[1] |
NGC 684 is a spiral galaxy approximately 135 million light-years away from Earth in the constellation of Triangulum.[1] It was discovered by William Herschel on October 26, 1786.[3] Edward Swift, Lewis' son, found this galaxy again on 18 Jan 1890 while "searching for Swift's Comet." and it was reported as a new object in list IX-6.[3]
NGC 684 is the largest member of a group of galaxies named after it (also known as LGG 32), which includes the galaxies NGC 670 and IC 1731.[4]
Two supernovae have been observed in NGC 684: