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From Wikipedia, the free encyclopedia

IC 3786
Observation data
ConstellationCanes Venatici
Right ascension191.90 degrees
Declination39.04 degrees
Redshift0.05472 0.00002
Heliocentric radial velocity16,036 km/s
Distance755 Mly (231.5 Mpc)
Apparent magnitude (V)20.16
Surface brightness22.9 mag/arcsec
Characteristics
TypeSbc
Other designations
PGC 2142309, 2MASX J12473689+3902461, ASK 507092.0, NPM1G +39.0301, SDSS J124736.89+390245.6, NSA 088286, 2MASS J12473689+3902461, LEDA 2142309

IC 3786 is a type Sbc[1] spiral galaxy in the Canes Venatici constellation.[2][3] It is located 755 million light-years[4] from the Milky Way and was discovered by Max Wolf on March 21, 1903.[5]

References

  1. ^ "HyperLeda -object description". atlas.obs-hp.fr. Retrieved 2024-04-26.
  2. ^ "Revised IC Data for IC 3786". spider.seds.org. Retrieved 2024-04-26.
  3. ^ Astronomy, Go. "IC 3786 | galaxy in Canes Venatici | IC List | GO ASTRONOMY". Go-Astronomy.com. Retrieved 2024-04-26.
  4. ^ "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2024-04-26.
  5. ^ "Index Catalog Objects: IC 3750 - 3799". cseligman.com. Retrieved 2024-04-26.
This page was last edited on 10 June 2024, at 15:14
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