In today's world, NGC 6087 is a topic that has become increasingly relevant and has captured the attention of a wide spectrum of society. Since its emergence, NGC 6087 has sparked debates, controversies and conflicting opinions, motivating experts and interested parties to deepen their study and understanding. In this article, we will explore the various dimensions and aspects related to NGC 6087, analyzing its impact in different fields and sectors, as well as its implications at an individual and collective level. Through an interdisciplinary approach, we will approach NGC 6087 from different perspectives, offering a comprehensive and updated vision on this topic that has aroused so much interest today.
NGC 6087 | |
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Observation data (J2000 epoch) | |
Right ascension | 16h 18m 48s[1] |
Declination | −57° 56′[1] |
Distance | ~3500LY (~1000pc) |
Apparent magnitude (V) | 5.4 |
Apparent dimensions (V) | 12′ |
Physical characteristics | |
Other designations | S Normae Cluster, Caldwell 89, Cr 300 |
Associations | |
Constellation | Norma |
NGC 6087 (also known as Caldwell 89 or the S Normae Cluster) is an open cluster of 40 or more[2][3] stars centered on the Cepheid variable S Normae in the constellation Norma. At a distance of about 3500 ly and covering a field of almost one quarter of a degree, the stars range from seventh- to eleventh-magnitude, the brightest being 6.5 magnitude S Normae. The aggregate visual magnitude of the cluster is about 5.4.
Spectral analysis of the radial motion of the stars confirm that S Normae is a member of the cluster,[3] and the period/luminosity relationship of Cepheid variables allows the distance to be determined with confidence.