NGC 3953 is a barred spiral galaxy located in the constellation Ursa Major. Its velocity with respect to the cosmic microwave background is 1,236±13 km/s, which corresponds to a Hubble distance of 59.4 ± 4.2 Mly (18.22 ± 1.29 Mpc).[1] However, 33 non-redshift measurements give a closer mean distance of 54.10 ± 1.93 Mly (16.588 ± 0.592 Mpc).[2] It was discovered by Pierre Méchain on 12 March 1781.[3][4][5]

NGC 3953
NGC 3953 captured in 2026
Observation data (J2000 epoch)
ConstellationUrsa Major
Right ascension11h 53m 49.0283s[1]
Declination+52° 19 36.480[1]
Redshift0.003502±0.00000200[1]
Heliocentric radial velocity1,050±1 km/s[1]
Distance54.10 ± 1.93 Mly (16.588 ± 0.592 Mpc)[1]
Group or clusterM109 Group
Apparent magnitude (V)10.8[1]
Characteristics
TypeSB(r)bc[1]
Size131,200 ly (40.24 kpc) (estimated)[1]
Apparent size (V)6.9′ × 3.5′[1]
Other designations
IRAS 11511+5236, 2MASX J11534902+5219355, UGC 6870, MCG +09-20-026, PGC 37306, CGCG 269-013[1]

NGC 3953 is known to exhibit an inner ring structure that encircles the bar. NGC 3953 is a member of the M109 Group, a large group of galaxies located within the constellation Ursa Major that may contain over 50 galaxies.[6][7][8][9]

Supernovae

edit
SN 2006bp

Two supernovae have been identified within NGC 3953:

References

edit
  1. 1 2 3 4 5 6 7 8 9 10 11 "Results for object NGC 3953". NASA/IPAC Extragalactic Database. Retrieved 2024-10-08.
  2. "Distance Results for NGC 3953". NASA/IPAC EXTRAGALACTIC DATABASE. NASA. Retrieved 22 February 2026.
  3. Henk Bril (2006). "Fortin – Other weird findings: The truth about the identity of M109". www.astrobril.nl: Astrohistorica. Retrieved 14 April 2025.
  4. Hartmut Frommert (2014). "Messier 109 and Messier 109B". SEDS Messier Catalog. Retrieved 14 April 2025.
  5. "NGC 3953 im Großen Bären (Ursa Major)". Spektrum der Wissenschaft (in German). 2024.
  6. R. B. Tully (1988). Nearby Galaxies Catalog. Cambridge: Cambridge University Press. ISBN 978-0-521-35299-4.
  7. P. Fouque; E. Gourgoulhon; P. Chamaraux; G. Paturel (1992). "Groups of galaxies within 80 Mpc. II – The catalogue of groups and group members". Astronomy and Astrophysics Supplement. 93: 211–233. Bibcode:1992A&AS...93..211F.
  8. A. Garcia (1993). "General study of group membership. II – Determination of nearby groups". Astronomy and Astrophysics Supplement. 100: 47–90. Bibcode:1993A&AS..100...47G.
  9. G. Giuricin; C. Marinoni; L. Ceriani; A. Pisani (2000). "Nearby Optical Galaxies: Selection of the Sample and Identification of Groups". Astrophysical Journal. 543 (1): 178–194. arXiv:astro-ph/0001140. Bibcode:2000ApJ...543..178G. doi:10.1086/317070. S2CID 9618325.
  10. Migliardi, M.; Dal Farra, E.; Kato, T.; Sano, Y. (2001). "Supernova 2001dp in NGC 3953". International Astronomical Union Circular (7683): 1. Bibcode:2001IAUC.7683....1M.
  11. "SN 2001dp". Transient Name Server. IAU. Retrieved 22 February 2026.
  12. "Results for object SN 2001dp". NASA/IPAC Extragalactic Database. Retrieved 2024-10-08.
  13. Nakano, S.; Itagaki, K. (2006). "Supernova 2006bp in NGC 3953". International Astronomical Union Circular (8700): 4. Bibcode:2006IAUC.8700....4N.
  14. "SN 2006bp". Transient Name Server. IAU. Retrieved 22 February 2026.
  15. "Results for object SN 2006bp". NASA/IPAC Extragalactic Database. Retrieved 2024-10-08.
edit