NGC 1992: Difference between revisions
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| name = NGC 1992 |
| name = NGC 1992 |
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| image = File:NGC 1992 DSS.jpg |
| image = File:NGC 1992 DSS.jpg |
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| caption = The |
| caption = The lenticular galaxy NGC 1992 |
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| epoch = [[J2000.0]] |
| epoch = [[J2000.0]] |
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| type = SO |
| type = SO |
Revision as of 10:28, 25 November 2017
NGC 1992 | |
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Observation data (J2000.0 epoch) | |
Constellation | Columba |
Right ascension | 05h 34m 31.8s[1] |
Declination | −30° 53′ 49″[1] |
Redshift | 0.035361 +/- 0.000150[2] |
Heliocentric radial velocity | 10601 +/- 45[2] |
Distance | 483 million |
Apparent magnitude (V) | 13.8[3] |
Apparent magnitude (B) | 14.65 [2] |
Characteristics | |
Type | SO |
Size | 1.10 x 0.7[2] |
Other designations | |
ESO 423- G 023, AM 0532-305, 2MASX J05343177-3053492, PGC 017466 [2] |
NGC 1992 (also known as PGC 17466) is a lenticular galaxy located in the Columba constellation. It was discovered by John Herschel on November 19, 1835.[4] It is about 483 million light years from the Milky Way, Its apparent magnitude is 14.65 and its size is 1.10 x 0.7 arc minutes.[2][3]
References
- ^ a b "Galaxy NGC 1992". DSO. Retrieved 22 November 2017.
- ^ a b c d e f "NGC 1992". NED. Retrieved 22 November 2017.
- ^ a b "Object: NGC 1992 (*)". SEDS. Retrieved 22 November 2017.
- ^ "NGC 1992". cseligman. Retrieved 22 November 2017.