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

NGC 3264 Group

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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

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References

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  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.
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