Astronomy:NGC 4141

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NGC 4141
NGC 4141 imaged by Legacy Surveys
Observation data (J2000 epoch)
ConstellationUrsa Major
Right ascension 12h 09m 47.3208s[1]
Declination+58° 50′ 57.066″[1]
Redshift0.006354±0.000009[1]
Helio radial velocity1,905±3 km/s[1]
Distance133.07 ± 10.76 Mly (40.800 ± 3.300 Mpc)[1]
Apparent magnitude (V)14.6g[1]
Characteristics
TypeSBcd[1]
Size~54,200 ly (16.62 kpc) (estimated)[1]
Apparent size (V)0.96′ × 0.74′[1]
Other designations
IRAS F12072+5907, UGC 7147, MCG+10-17-152, PGC 38669[1]

NGC 4141 is a barred spiral galaxy in the constellation of Ursa Major. Its velocity with respect to the cosmic microwave background is 2,051±11 km/s, which corresponds to a Hubble distance of 98.7 ± 6.9 Mly (30.25 ± 2.12 Mpc).[1] However, two non-redshift measurements give a farther mean distance of 133 ± 11 Mly (40.8 ± 3.3 Mpc).[2] It was discovered by German-British astronomer William Herschel on 17 April 1789.[3][4]

NGC 4141 is listed as having an active galactic nucleus.[5]

Supernovae

Two supernovae has been observed in NGC 4141:

  • SN 2008X (Type II-P, mag. 17.6) was discovered by Scottish amateur astronomer Tom Boles, and independently by the Lick Observatory Supernova Search (LOSS), on 7 February 2008.[6][7]
  • SN 2009E (Type II-P, mag. 17.8) was discovered by Tom Boles on 3 January 2009.[8][9]

See also

References

Coordinates: Sky map 12h 09m 47.3208s, +58° 50′ 57.066″