![]() | The topic of this articlemay not meet Wikipedia'snotability guideline for astronomical objects. Please help to demonstrate the notability of the topic by citingreliable secondary sources that areindependent of the topic and provide significant coverage of it beyond a mere trivial mention. If notability cannot be shown, the article is likely to bemerged,redirected, ordeleted. Find sources: "NGC 2494" – news ·newspapers ·books ·scholar ·JSTOR(April 2024) (Learn how and when to remove this message) |
NGC 2494 | |
---|---|
![]() PAN-STARRS image of NGC 2494 | |
Observation data (J2000epoch) | |
Constellation | Monoceros |
Right ascension | 07h 59m 07.1188s[1] |
Declination | −00° 38′ 16.626″[1] |
Redshift | 0.011955 0.000103 |
Heliocentric radial velocity | 3,594 km/s |
Distance | 183Mly (56.1 Mpc) |
Apparent magnitude (V) | 13.4 |
Characteristics | |
Type | (R')SB0/a(rs)[1] |
Size | 58,000 ly |
Other designations | |
IRAS F07565-0030,IC 487,UGC 4141,LEDA 22377,MCG +00-21-001,PGC 22377,CGCG 003-002 |
NGC 2494 is a barredlenticular galaxy located in theMonoceros constellation.[2] It is 183 million light-years away and about 58,000 light-years in diameter.[1]
NGC 2494 was discovered on February 6 in 1864 byAlbert Marth who listed it as NGC 2494. Subsequently, on February 3, 1888, it was observed again byLewis Swift who gave it the designation as IC 487.[3] It has a broadH II region[1] and amagnitude brightness of 12.60.[4]
![]() | Thislenticular galaxy article is astub. You can help Wikipedia byexpanding it. |