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EntityQ1148401· pop 30· linked from 521 articles

galaxy

Astronomical data · SIMBAD

Object type
GiG
Distance
2,414 light-years
Redshift
z = 0.009363280866388157
Coordinates
RA 306.1169° · Dec -43.6534°
View on SIMBAD →

via SIMBAD · CDS Strasbourg

Key facts

Constellation
Sagittarius
Right ascension
20 24 28.067
Declination
−43 ° 39 ′ 12.42 ″
Redshift
0.009300 ± 0.000023
Heliocentric radial velocity
2 793 .9 km/s
Distance
124 Mly (38.0 Mpc )
Group or cluster
LGG 434
Apparent magnitude v
10.93 ± 0.18
Apparent magnitude b
11.64 ± 0.18
Type
SA(r)b
Size
~334,800 ly (102.64 kpc ) (estimated)
Apparent size v
3.55 ′ × 2.69 ′

via Wikipedia infobox

~2 min read

Encyclopedic overview

NGC 6902 is an unbarred spiral galaxy located in the southern constellation of Sagittarius at an approximate distance of 124 million light-years (38.0 Mpc). NGC 6902 was discovered on September 2, 1836 by English astronomer John Herschel. In his New General Catalogue, Danish astronomer J. L. E. Dreyer described it as faint, considerably small, round, brighter middle. It is a member of the small NGC 6092 group of galaxies; the LGG 434 group.

The morphological classification of NGC 6902 is SA(r)b, indicating an unbarred spiral galaxy (SA) with an inner ring (r) and somewhat tightly wound arms (b). As the two arms extend outward, they transition into a complex system of filamentary arms. The galaxy has an angular size of 3.55′ × 2.69′ in the optical band. The galactic plane is inclined at an angle of 38±5° to the line of sight from the Earth. NGC 6902 has a high abundance of neutral hydrogen; about three times greater than a typical galaxy of this class. The ring structure is undergoing extensive star formation. Although classed as unbarred, there is a small bar of stars inside the ring.

Excerpted from Wikipedia’s “Q1148401” article, available under the CC BY-SA 4.0 licence.