In this article we will explore in depth the topic of NGC 656, which has been the subject of interest and debate in various spheres of society. NGC 656 has aroused the interest of experts, academics, professionals and the general public, generating a wide range of opinions and perspectives on its importance, implications and relevance today. Through a comprehensive analysis, we will examine the fundamental aspects of NGC 656, its impact in different contexts, and the possible implications it has for the future. Likewise, we will address various approaches and theories that have been developed around NGC 656, with the aim of offering a comprehensive and multidimensional vision of this topic.
NGC 656 | |
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![]() SDSS image of NGC 656 | |
Observation data (J2000 epoch) | |
Constellation | Pisces |
Right ascension | 01h 42m 27.229s[1] |
Declination | +26° 08′ 35.06″[1] |
Redshift | 0.013129[2] |
Heliocentric radial velocity | 3910 km/s[2] |
Distance | 174.8 Mly (53.60 Mpc)[3] |
Apparent magnitude (B) | 13.50[2] |
Characteristics | |
Type | SB0[2][3] |
Other designations | |
UGC 1194, MCG +04-05-002, PGC 6293[2] |
NGC 656 is a barred lenticular galaxy located in the Pisces constellation about 175 million light-years from the Milky Way. It was discovered by the Prussian astronomer Heinrich d'Arrest in 1865.[4][5][6]