Astronomy:NGC 6027d

From HandWiki
NGC 6027d
NGC 6027d imaged by the Hubble Space Telescope
Observation data (J2000 epoch)
ConstellationSerpens
Right ascension 15h 59m 12.9156s[1]
Declination+20° 45′ 35.535″[1]
Redshift0.066089[1]
Helio radial velocity19813 ± 35 km/s[1]
Distance957.5 ± 67.1 Mly (293.58 ± 20.56 Mpc)[1]
Apparent magnitude (V)16.5[1]
Characteristics
TypeSB(s)bc[1]
Size~181,600 ly (55.68 kpc) (estimated)[1]
Apparent size (V)0′.2 × 0′.2[1]
Other designations
UGC 10116 NED05, MCG+04-38-009, PGC 56580[1]

NGC 6027d is a face-on barred spiral galaxy located approximately 877 million light-years (269 Mpc) away in the constellation Serpens.[2] Although it appears visually within Seyfert's Sextet (HCG 79), high-resolution spectroscopy demonstrates that NGC 6027d is an unassociated background galaxy located nearly five times further away than the core interacting group.[2] The galaxy has an apparent visual magnitude of 16.5.[3]

Physical Characteristics

NGC 6027d exhibits a recessional velocity of approximately 19,813 km/s, significantly higher than the 4,350 km/s mean velocity of the interacting cluster core.[3] Because it lies in the far background along the same line of sight, NGC 6027d does not experience gravitational interactions or tidal disruptions from the members of Seyfert's Sextet.[2]

Supernovae

One supernova has been recorded in NGC 6027d. Supernova SN 1998fe was detected on July 19, 1998, by the Lick Observatory Supernova Search.[4] Its type is unknown, and it reached a peak visual magnitude of 18.[5] Its type is unknown, and had a peak visual magnitude of 18.[6]

See also

References

Template:NGC objects: 6001-7000 Coordinates: Sky map 15h 59m 12.9156s, +20° 45′ 35.535″