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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°
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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

Wikidata facts

Instance of
spiral galaxy
Constellation
Sagittarius
Distance from Earth
41.7
Image
NGC 6902 GALEX WikiSky.jpg
Show 11 more facts
Commons category
NGC 6902
discoverer or inventor
John Frederick William Herschel
time of discovery or invention
1836-09-02
catalog code
Gaia DR2 6678974930431764096
epoch
J2000.0
apparent magnitude
8.612
galaxy morphological type
Sa
redshift
0.009300
right ascension
306.11693924821860
declination
-43.65345276812860
radial velocity
2781

via Wikidata · CC0

~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.