Astronomy:IC 438

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IC 438
A large spiral galaxy seen close-up. The left side of the image shows the galaxy's core and its tightly-curled inner spiral arms. On the right side, one of the arms reaches down from above, curving across the dark background. There is a bright star inside the arc of the arm, and a couple more next to the galaxy.
IC 438 imaged by the Hubble Space Telescope in 2021
Observation data (J2000 epoch)
ConstellationLepus
Right ascension 05h 53m 00.0676s[1]
Declination−17° 52′ 33.684″[1]
Redshift0.004256±0.000006[1]
Helio radial velocity3,123±4 km/s[1]
Distance136.45 ± 4.29 Mly (41.835 ± 1.314 Mpc)[1]
Group or clusterIC 438 Group (LGG 134)
Apparent magnitude (V)12.74[1]
Characteristics
TypeSA(rs)c[1]
Size~155,100 ly (47.55 kpc) (estimated)[1]
Apparent size (V)2.8′ × 2.1′[1]
Other designations
ESO 555- G 009, IRAS 05508-1753, MCG-03-15-025, PGC 18047[1]

IC 438 is a spiral galaxy in the constellation of Lepus. Its velocity with respect to the cosmic microwave background is 3,199±6 km/s, which corresponds to a Hubble distance of 153.9 ± 10.8 Mly (47.18 ± 3.30 Mpc).[1] However, 17 non-redshift measurements give a much closer distance of 136.45 ± 4.29 Mly (41.835 ± 1.314 Mpc).[2] It was discovered by American astronomer Lewis Swift on 7 January 1891.[3][4]

IC 438 is a Seyfert I Galaxy, i.e. it has a quasar-like nucleus with very high surface brightnesses whose spectra reveal strong, high-ionisation emission lines, but unlike quasars, the host galaxy is clearly detectable.[5]

IC 438 Group

According to A.M. Garcia, IC 438 is one of five members of the IC 438 galaxy group (also known as LGG 134), which includes IC 2143, UGCA 113, MCG -03-15-021, and ESO 555- G 005.[6]

Supernovae

Three supernovae have been observed in IC 438:

See also

  • List of IC objects

References

  1. 1.00 1.01 1.02 1.03 1.04 1.05 1.06 1.07 1.08 1.09 1.10 "Results for object IC 0438". NASA and Caltech. https://ned.ipac.caltech.edu/byname?objname=IC+0438. 
  2. "Distance Results for IC 438". NASA. https://ned.ipac.caltech.edu/cgi-bin/nDistance?name=IC+438. 
  3. Seligman, Courtney. "Index Catalogue Objects: IC 438". https://cseligman.com/text/atlas/ic4.htm#ic438. 
  4. Swift, Lewis (1892). "Catalogue No. 10 of Nebulae discovered at the Warner Observatory". Astronomische Nachrichten 129 (24): 361–364. doi:10.1002/asna.18921292402. Bibcode1892AN....129..361S. 
  5. Chen, Yan-Ping; Zaw, Ingyin; Farrar, Glennys R.; Elgamal, Sana (2022). "A Uniformly Selected, Southern-sky 6dF, Optical AGN Catalog". The Astrophysical Journal Supplement Series 258 (2): 29. doi:10.3847/1538-4365/ac4157. Bibcode2022ApJS..258...29C. 
  6. Garcia, A. M. (1993). "General study of group membership. II. Determination of nearby groups". Astronomy and Astrophysics Supplement Series 100: 47. Bibcode1993A&AS..100...47G. 
  7. "SN 1997B". IAU. https://www.wis-tns.org/object/1997B. 
  8. Gabrijelcic, A.; Valles, P.; Benetti, S.; Lidman, C. (1997). Green, Daniel W. E.. ed. "Supernova 1997B in IC 438". International Astronomical Union Circular (6535): 1. Bibcode1997IAUC.6535....1G. http://www.cbat.eps.harvard.edu/iauc/06500/06535.html#Item1. 
  9. "SN 2016blx". IAU. https://www.wis-tns.org/object/2016blx. 
  10. "SN 2017gbb". IAU. https://www.wis-tns.org/object/2017gbb.