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NGC 3197

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NGC 3197
NGC 3197 (left) with PGC 213677 (right) imaged by Legacy Surveys
Observation data (J2000 epoch)
ConstellationDraco
Right ascension10h 14m 27.7181s[1]
Declination+77° 49′ 13.427″[1]
Redshift0.027069±0.0000120[1]
Heliocentric radial velocity8,115±4 km/s[1]
Distance348.99 ± 4.98 Mly (107.000 ± 1.528 Mpc)[1]
Apparent magnitude (V)14.34[1]
Characteristics
TypeSbc[1]
Size~181,900 ly (55.77 kpc) (estimated)[1]
Apparent size (V)1.3′ × 1.0′[1]
Other designations
2MASX J10142763+7749129, UGC 5500, MCG +13-08-009, PGC 29870, CGCG 350-045[1]

NGC 3197 is a spiral galaxy in the constellation of Draco. Its velocity with respect to the cosmic microwave background is 8,146±4 km/s, which corresponds to a Hubble distance of 391.9 ± 27.4 Mly (120.15 ± 8.41 Mpc).[1] However, three non-redshift measurements give a closer mean distance of 348.99 ± 4.98 Mly (107.000 ± 1.528 Mpc).[2] It was discovered by German-British astronomer William Herschel on 2 April 1801.[3][4]

Supernovae

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Two supernovae have been observed in NGC 3197:

See also

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References

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  1. ^ a b c d e f g h i j k "Results for object NGC 3197". NASA/IPAC Extragalactic Database. NASA and Caltech. Retrieved 6 February 2026.
  2. ^ "Distance Results for NGC 3197". NASA/IPAC EXTRAGALACTIC DATABASE. NASA. Retrieved 6 February 2026.
  3. ^ Herschel, William (1802). "Catalogue of 500 New Nebulae, Nebulous Stars, Planetary Nebulae, and Clusters of Stars; with Remarks on the Construction of the Heavens". Philosophical Transactions of the Royal Society of London. 92: 477–528. Bibcode:1802RSPT...92..477H. doi:10.1098/rstl.1802.0021.
  4. ^ Seligman, Courtney. "New General Catalogue Objects: NGC 3197". Celestial Atlas. Retrieved 6 February 2026.
  5. ^ Puckett, T.; Tigner, J. (2005). "Supernovae 2005kv-2005kx". International Astronomical Union Circular (8635): 3. Bibcode:2005IAUC.8635....3P.
  6. ^ "SN 2005kx". Transient Name Server. IAU. Retrieved 6 February 2026.
  7. ^ "SN 2022xqp". Transient Name Server. IAU. Retrieved 6 February 2026.
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