In this article, we will explore the topic of NGC 6055 in depth, analyzing its origins, evolution, impact and possible future prospects. NGC 6055 has been the subject of interest and debate throughout history, influencing various aspects of society, culture and politics. Throughout the next sections, we will delve into its meaning, its implications and its relevance in the current context, shedding light on the various facets that make up this phenomenon. Additionally, we will examine different approaches and opinions to offer a comprehensive and balanced view, providing the reader with a broader and deeper understanding of NGC 6055.
NGC 6055 | |
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![]() SDSS image of NGC 6055. | |
Observation data (J2000 epoch) | |
Constellation | Hercules |
Right ascension | 16h 05m 32.5s[1] |
Declination | 18° 09′ 34″[1] |
Redshift | 0.037773[1] |
Heliocentric radial velocity | 11324 km/s[1] |
Distance | 137 Mpc (447 Mly)[1] |
Group or cluster | Hercules Cluster |
Apparent magnitude (V) | 14.7[1] |
Characteristics | |
Type | (R)SAB0^+[1] |
Size | ~160,000 ly (48 kpc)[1] (estimated)[1] |
Apparent size (V) | 1.0 x 0.6[1] |
Other designations | |
CGCG 108-123, MCG 3-41-101, PGC 57076, UGC 10191[1] |
NGC 6055 is a barred[2] lenticular galaxy located about 450 million light-years away[3] in the constellation Hercules.[4] The galaxy was discovered by astronomer Lewis Swift on June 8, 1886.[5][6] It also a member of the Hercules Cluster[7][8] and is a LINER galaxy.[9]