In this article we are going to delve into the fascinating world of NGC 1725, exploring its origins, evolution and relevance today. NGC 1725 has been the subject of interest and debate for many years, and its influence extends to various areas of society. Along these lines, we will analyze in depth the different aspects that make NGC 1725 such an exciting topic, from its impact on popular culture to its importance in the academic and scientific field. Get ready to discover all the fascinating aspects of NGC 1725 and immerse yourself in a journey that will lead you to better understand its relevance in today's world.
NGC 1725 | |
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Observation data (J2000 epoch) | |
Constellation | Eridanus |
Right ascension | 04h 59m 22.9s[1] |
Declination | −11° 07′ 56″[1] |
Redshift | 0.012956[1] |
Heliocentric radial velocity | 3 884 ± 42 km/s[1] |
Galactocentric velocity | 3 772 ± 42 km/s[1] |
Distance | 172.8 Mly (53.0 Mpc) h−1 0.73 [1] |
Apparent magnitude (B) | 13[2] |
Characteristics | |
Type | S0[1] |
Size | 18.7 × 14.4 h−1 0.73 kpc[1] |
Other designations | |
MCG -02-13-028, PGC 16488[2] |
NGC 1725 is a lenticular galaxy in the constellation Eridanus. The galaxy is listed in the New General Catalogue. It was discovered on November 10, 1885 by the astronomer Edward Emerson Barnard.[3]
In 2009, a type Ia supernova was detected within NGC 1725. It was subsequently designated SN 2009F.[4]