Back NGC 513 Arabic NGC 513 (مجره) ARZ NGC 513 AST NGC 513 Azerbaijani NGC 513 Byelorussian NGC 513 BS NGC 513 CE NGC 513 Czech NGC 513 German NGC 513 DIQ
| NGC 513 | |
|---|---|
 NGC 513 (NASA/ESA HST) | |
| Observation data (J2000[1] epoch) | |
| Constellation | Andromeda[2] |
| Right ascension | 01h 24m 26.8s[3] |
| Declination | +33° 47′ 58″[3] |
| Redshift | 0.019560 ± 0.000357[1] |
| Heliocentric radial velocity | (5807 ± 107) km/s[1] |
| Distance | 262 Mly[4] |
| Apparent magnitude (V) | 12.9[2] |
| Apparent magnitude (B) | 13.6[2] |
| Characteristics | |
| Type | Sc[2] |
| Apparent size (V) | 0.9' × 0.6'[2] |
| Other designations | |
| PGC 5174, UGC 953, GC 297, MCG +06-04-016, 2MASS J01242680+3347585, IRAS F01216+3332[1][5] | |
NGC 513, also occasionally referred to as PGC 5174 or UGC 953, is a spiral galaxy in the constellation Andromeda.[2] It is located approximately 262 million light-years from the Solar System[4] and was discovered on 13 September 1784 by astronomer William Herschel.[5]
- ^ a b c d "NGC 513". Retrieved 2017-12-09.
- ^ a b c d e f "Revised NGC Data for NGC 513". spider.seds.org. Retrieved 2017-10-05.
- ^ a b "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2017-10-05.
- ^ a b An object's distance from Earth can be determined using Hubble's law: v=Ho is Hubble's constant (70±5 (km/s)/Mpc). The relative uncertainty Δd/d divided by the distance is equal to the sum of the relative uncertainties of the velocity and v=Ho
- ^ a b "New General Catalog Objects: NGC 500 - 549". cseligman.com. Retrieved 2017-10-16.