NGC 2688
Appearance
This article, NGC 2688, has recently been created via the Articles for creation process. Please check to see if the reviewer has accidentally left this template after accepting the draft and take appropriate action as necessary.
Reviewer tools: Inform author |
NGC 2688 | |
---|---|
Observation data | |
Constellation | Ursa Major |
Redshift | 0.05204 0.00001 |
Heliocentric radial velocity | 15,190 km/s |
Distance | 758 Mly (232.4 Mpc) |
Apparent magnitude (V) | 15.8 |
Characteristics | |
Type | Sb |
Size | 154,000 ly |
Other designations | |
PGC 25048, 2MASX J08551161+4907218, MCG+08-16-040, SDSS J085511.60+490721.3 |
NGC 2688 is a spiral galaxy located in Ursa Major.[1][2][3] It is located 758 million light-years away from the solar system and is moving away at a speed of 15,190 km/s.[4] NGC 2688 was found by R.J. Mitchell who was an Irish astronomer and assistant to William Parsons.[5] When Mitchell first saw the object, he commented it as very small and faint. According to Professor Seligman, the galaxy is classified to be a lenticular galaxy rather than a spiral galaxy.[5]
References
- ^ "NGC 2688 - Spiral Galaxy in Ursa Major | TheSkyLive.com". theskylive.com. Retrieved 2024-04-17.
- ^ "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2024-04-17.
- ^ "NGC 2688". simbad.u-strasbg.fr. Retrieved 2024-04-17.
- ^ Guide, Universe (02-07-2022T20:30:12). "NGC 2688 Galaxy Facts". Universe Guide. Retrieved 2024-04-17.
{{cite web}}
: Check date values in:|date=
(help) - ^ a b "New General Catalog Objects: NGC 2650 - 2699". cseligman.com. Retrieved 2024-04-17.