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NGC 2012

From Wikipedia, the free encyclopedia
Large spiral galaxy in Mensa
NGC 2012
NGC 2012, as photographed during theDigitized Sky Survey (DSS2)
Observation data (J2000epoch)
ConstellationMensa
Right ascension05h 22m 35s
Declination-79° 51’ 06”
Distance236.137Mly (51.66 Mpc)
Apparent magnitude (V)10.58
Apparent magnitude (B)14.49
Surface brightness23.29 mag/arcsec2
Characteristics
TypeE-SO
Apparent size (V)1 arcmin
Notable featuresN/A
Other designations
Leda 17194

NGC 2012 is a large lenticular galaxy in theConstellation Mensa.[1] It was discovered byJohn Herschel in 1836. With its distance from the Earth being over 236 millionlight years,[2] NGC 2012 is not visible to the naked eye, and a largetelescope is needed. A probe has never been sent out to study the galaxy.[3]

Discovery

[edit]

PolymathJohn Herschel observed the galaxy in 1836, and it was then added to theNew General Catalog (NGC). The galaxy itself is a relatively long distance from Earth, making Herschel's find very uncommon for the time period.

References

[edit]
  1. ^"NGC 2012".spider.seds.org. Retrieved2024-03-19.
  2. ^"Your NED Search Results".ned.ipac.caltech.edu. Retrieved2024-03-19.
  3. ^"NGC 2012 - Elliptical/Spiral Galaxy in Mensa | TheSkyLive.com".theskylive.com. Retrieved2024-03-19.
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