NGC 3353

NGC 3353
NGC 3353 imaged by the Hubble Space Telescope
Observation data (J2000 epoch)
ConstellationUrsa Major
Right ascension10h 45m 22.296s[1]
Declination+55° 57′ 39.24″[1]
Redshift0.003139[1]
Heliocentric radial velocity941 ± 1 km/s[1]
Distance53.3 ± 3.8 Mly (16.35 ± 1.16 Mpc)[1]
Group or clusterNGC 3264 Group (LGG 201)
Apparent magnitude (V)12.8[1]
Characteristics
TypeSb? pec[1]
Size~27,300 ly (8.36 kpc) (estimated)[1]
Other designations
IRAS 10422+5613, UGC 5860, MCG +09-18-022, Mrk 35, PGC 32103, CGCG 267-009[1]

NGC 3353 is an Intermediate spiral galaxy located in the constellation of Ursa Major.[2][3]Its velocity with respect to the cosmic microwave background is 1108 ± 12 km/s, which corresponds to a Hubble distance of 53.3 ± 3.8 Mly (16.35 ± 1.16 Mpc).[1] In addition, four non-redshift measurements give a distance of 62.46 ± 2.66 Mly (19.150 ± 0.817 Mpc).[4] NGC 3353 was discovered on March 18, 1790, by William Herschel,[5] a German born British astronomer.[6]

NGC 3353 is a galaxy whose nucleus shines in the ultraviolet range. It is listed in the Markarian catalogue as Mrk 35.

NGC 3264 Group

NGC 3353 is part of the NGC 3264 group (also known as LGG 201), which includes at least five other members: NGC 3206, NGC 3220, NGC 3264, UGC 5848, and UGCA 211.[7]

See also

References

  1. ^ a b c d e f g h i j "Results for object NGC 3353". NASA/IPAC Extragalactic Database. NASA and Caltech. Retrieved November 25, 2024.
  2. ^ "Revised NGC Data for NGC 3353". spider.seds.org. Retrieved October 27, 2023.
  3. ^ Ford, Dominic. "NGC3353 (Galaxy)". In-The-Sky.org. Retrieved October 27, 2023.
  4. ^ "Distance Results for NGC 3353". NASA/IPAC EXTRAGALACTIC DATABASE. NASA. Retrieved November 25, 2024.
  5. ^ "New General Catalog Objects: NGC 3350 - 3399". cseligman.com. Retrieved October 27, 2023.
  6. ^ "William Herschel | Biography, Education, Telescopes, & Facts | Britannica". www.britannica.com. Retrieved October 27, 2023.
  7. ^ Garcia, A. M. (1993). "General study of group membership. II. Determination of nearby groups". Astronomy and Astrophysics Supplement Series. 100: 47. Bibcode:1993A&AS..100...47G.