NGC 684

NGC 684
NGC 684 (SDSS)
Observation data (J2000.0 epoch)
ConstellationTriangulum
Right ascension01h 50m 14.0407s [1]
Declination+27° 38 44.472 [1]
Redshift0.011798 [1]
Heliocentric radial velocity3537 ± 1 km/s [1]
Distance135.03 ± 3.13 Mly (41.400 ± 0.960 Mpc)[1]
Group or clusterNGC 684 group (LGG 32)
Apparent magnitude (V)12.50 [2]
Apparent magnitude (B)13.30 [2]
Characteristics
TypeSb edge-on [1]
Size~137,500 ly (42.15 kpc) (estimated)[1]
Apparent size (V)3.2′ × 0.6′[1]
Other designations
IRAS 01474+2724, IC 165, UGC 1292, MCG +04-05-017, PGC 6759, CGCG 482-022[1]

NGC 684 is a spiral galaxy approximately 135 million light-years away from Earth in the constellation of Triangulum.[1] It was discovered by William Herschel on October 26, 1786.[3] Edward Swift, Lewis' son, found this galaxy again on 18 Jan 1890 while "searching for Swift's Comet." and it was reported as a new object in list IX-6.[3]

NGC 684 Group

NGC 684 is the largest member of a group of galaxies named after it (also known as LGG 32), which includes the galaxies NGC 670 and IC 1731.[4]

Supernovae

Two supernovae have been observed in NGC 684:

See also

References

  1. 1 2 3 4 5 6 7 8 9 10 "Results for object NGC 0684". NASA/IPAC Extragalactic Database. NASA and Caltech. Retrieved 4 December 2017.
  2. 1 2 "Revised NGC Data for NGC 684". spider.seds.org. Retrieved December 9, 2017.
  3. 1 2 "Data for NGC 684". www.astronomy-mall.com. Retrieved December 9, 2017.
  4. 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.
  5. "SN 2021ass". Transient Name Server. IAU. Retrieved 4 September 2024.
  6. "SN 2025aml". Transient Name Server. IAU. Retrieved 31 January 2025.
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