NGC 6902

NGC 6902
NGC 6902 imaged by SPECULOOS
Observation data (J2000 epoch)
ConstellationSagittarius
Right ascension20h 24m 28.067s
Declination−43° 39 12.42
Redshift0.009300±0.000023
Heliocentric radial velocity2793.9 km/s
Distance124 Mly (38.0 Mpc)
Group or clusterLGG 434
Apparent magnitude (V)10.93±0.18
Apparent magnitude (B)11.64±0.18
Characteristics
TypeSA(r)b
Size~334,800 ly (102.64 kpc) (estimated)
Apparent size (V)3.55 × 2.69
Other designations
Gaia DR2 6678974930431764096, IRAS 20210-4348, F20210-4348, 2MASX J20242813-4339127, NGC 6902, IC 4948, LEDA 64632, MCG -07-42-002, PGC 64632

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.

One supernova has been observed in NGC 6902: SN 2024uwq (type Ic-BL, mag. 17.4).