| NGC 6285 | |
|---|---|
 NGC 6285 (below) and NGC 6286 (above) as seen through the 0.81 m Schulman Telescope at Mount Lemmon Observatory. | |
| Observation data (J2000 epoch) | |
| Constellation | Draco |
| Right ascension | 16h 58m 24.0s [1] |
| Declination | +58° 57′ 21″ [1] |
| Redshift | 0.018983±0.000160 [1] |
| Heliocentric radial velocity | 5691±48 km/s [1] |
| Galactocentric velocity | 5880±49 km/s [1] |
| Distance | 262 million light years (80.2 million parsecs) |
| Apparent magnitude (V) | 13.6 [2] |
| Characteristics | |
| Type | S0-a |
| Size | 91,000 light years |
| Apparent size (V) | 1.20′ × 0.7′ [2] |
| Other designations | |
| MCG 10-24-81, ZWG 299.37, ARP 293, PGC 59344 and KAZ 111 | |
References: NASA/IPAC extragalactic datatbase, http://spider.seds.org/ | |
NGC 6285 is an interacting spiral galaxy located in the constellation Draco. It is classified as S0-a in the galaxy morphological classification scheme and was discovered by the American astronomer Lewis A. Swift in 1886. [3] NGC 6285 is located at about 262 million light years away from Earth. NGC 6285 and NGC 6286 form a pair of interacting galaxies, with tidal distortions, categorized as Arp 293 in the Arp Atlas of Peculiar Galaxies. [1] [2] [4]
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