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NGC 5235

From Wikipedia, the free encyclopedia
NGC 5235
The barred spiral galaxy NGC 5235.
Observation data (J2000 epoch)
ConstellationVirgo
Right ascension13h 36m 01.4057s[1]
Declination+06° 35′ 07.272″[1]
Redshift0.021949[1]
Heliocentric radial velocity6580 ± 10 km/s[1]
Distance330.5 ± 23.2 Mly (101.34 ± 7.10 Mpc)[1]
Apparent magnitude (V)14.2[1]
Characteristics
TypeSB[1]
Size~109,100 ly (33.45 kpc) (estimated)[1]
Apparent size (V)1.2' x 0.5'[1]
Other designations
IRAS 13335+0650, 2MASX J13360139+0635076, UGC 8582, MCG +01-35-012, PGC 47984, CGCG 045-036[1]

NGC 5235 is an intermediate spiral galaxy in the constellation of Virgo. Its velocity with respect to the cosmic microwave background is 6871 ± 23 km/s, which corresponds to a Hubble distance of 101.34 ± 7.10 Mpc (∼330 million light-years).[1] It was discovered by German-British astronomer William Herschel on 13 April 1784.[2]

In the same area of the sky are the galaxies NGC 5210, NGC 5224, and NGC 5239, among others.

One supernova has been observed in NGC 5235: SN 2024grb (type Ia, mag. 18.3).[3]

See also

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References

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  1. ^ a b c d e f g h i j k "NASA/IPAC Extragalactic Database". Results for NGC 5235. Retrieved 2 August 2024.
  2. ^ Celestial Atlas entry for NGC 5235. Retrieved 2 August 2024.
  3. ^ Transient Name Server entry for SN 2024grb. Retrieved 2 August 2024.
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