| NGC 525 | |
|---|---|
 NGC 525 as seen on SDSS | |
| Observation data (J2000[1] epoch) | |
| Constellation | Pisces[2] |
| Right ascension | 01h 24m 52.9s[3] |
| Declination | +09° 42′ 12″[3] |
| Redshift | 0.007158 ± 0.000167[1] |
| Heliocentric radial velocity | (2138 ± 50) km/s[1] |
| Distance | 95.6 Mly[4] |
| Apparent magnitude (V) | 13.3[2] |
| Apparent magnitude (B) | 14.3[2] |
| Characteristics | |
| Type | S0[2] |
| Apparent size (V) | 1.5' × 0.7'[2] |
| Other designations | |
| PGC 5232, UGC 972, MGC +01-04-054, 2MASS J01245290+09421164[1][5] | |
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NGC 525, also occasionally referred to as PGC 5232 or UGC 972, is a lenticular galaxy located approximately 95.6 million light-years from the Solar System[4] in the constellation Pisces.[2] It was discovered on 25 September 1862 by astronomer Heinrich d'Arrest.[5]
- ^ a b c d "NGC 525". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2017-12-09.
- ^ a b c d e f "Revised NGC Data for NGC 525". 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.