NGC 1385

NGC 1385
The barred spiral galaxy NGC 1385, imaged by the Hubble Space Telescope.
Observation data (J2000 epoch)
ConstellationFornax
Right ascension03h 37m 28.848s[1]
Declination−24° 30′ 01.076″[1]
Redshift0.004993 [1]
Heliocentric radial velocity1497 ± 4 km/s[1]
Distance66.4 ± 4.7 Mly (20.37 ± 1.43 Mpc)[1]
Apparent magnitude (V)10.9[1]
Characteristics
TypeSB(s)cd[1]
Size~94,000 ly (28.82 kpc) (estimated)[1]
Apparent size (V)3.6' x 2.2'[1]
Other designations
IRAS 03353-2439, 2MASX J10214758+5655494, MCG -04-09-036, PGC 13368, ESO 482-016[1]

NGC 1385 is a barred spiral galaxy in the constellation of Fornax. Its velocity with respect to the cosmic microwave background is 1381 ± 9 km/s, which corresponds to a Hubble distance of 20.37 ± 1.43 Mpc (∼66.5 million light-years).[1] In addition, 30 non redshift measurements give a distance of 15.999 ± 12.131 Mpc (~52.2 million light-years).[2] The galaxy was discovered by German-British astronomer William Herschel on 17 November 1784.[3][4]

Although no supernovae have yet been observed in NGC 1385, the astronomical transient AT 2020pju was discovered on 18 June 2020. Spectral analysis revealed the star to be a luminous blue variable.[5]

In 2024, NGC 1385 was imaged by James Webb Space Telescope as part of Physics at High Angular Project resolution in Nearby GalaxieS (PHANGS) project, studying phases of star formations.[6]

  1. ^ a b c d e f g h i j k "NASA/IPAC Extragalactic Database". Results for NGC 1385. Retrieved 15 August 2024.
  2. ^ "Distance Results for NGC 1385". NASA/IPAC EXTRAGALACTIC DATABASE. NASA. Retrieved 15 August 2024.
  3. ^ Seligman, Courtney. "NGC 1385". Celestial Atlas. Retrieved 15 August 2024.
  4. ^ Lazaro, Enrico de (2023-11-13). "Hubble Views Barred Spiral Galaxy NGC 1385 | Sci.News". Sci.News: Breaking Science News. Retrieved 2024-08-16.
  5. ^ "AT 2020pju". Transient Name Server. IAU. Retrieved 15 August 2024.
  6. ^ [email protected]. "NGC 1385 | ESA/Webb". esawebb.org. Retrieved 2024-08-16.