Jump to content

NGC 1992: Difference between revisions

From Wikipedia, the free encyclopedia
Content deleted Content added
stubsort
m double star → lenticular galaxy
Line 2: Line 2:
| name = NGC 1992
| name = NGC 1992
| image = File:NGC 1992 DSS.jpg
| image = File:NGC 1992 DSS.jpg
| caption = The double star NGC 1992
| caption = The lenticular galaxy NGC 1992
| epoch = [[J2000.0]]
| epoch = [[J2000.0]]
| type = SO
| type = SO

Revision as of 10:28, 25 November 2017

NGC 1992
The lenticular galaxy NGC 1992
Observation data (J2000.0 epoch)
ConstellationColumba
Right ascension05h 34m 31.8s[1]
Declination−30° 53′ 49″[1]
Redshift0.035361 +/- 0.000150[2]
Heliocentric radial velocity10601 +/- 45[2]
Distance483 million
Apparent magnitude (V)13.8[3]
Apparent magnitude (B)14.65 [2]
Characteristics
TypeSO
Size1.10 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

  1. ^ a b "Galaxy NGC 1992". DSO. Retrieved 22 November 2017.
  2. ^ a b c d e f "NGC 1992". NED. Retrieved 22 November 2017.
  3. ^ a b "Object: NGC 1992 (*)". SEDS. Retrieved 22 November 2017.
  4. ^ "NGC 1992". cseligman. Retrieved 22 November 2017.