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NGC 167

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Spiral galaxy in the constellation Cetus
NGC 167
NGC 167NGC 167 with DECam
Observation data (J2000 epoch)
ConstellationCetus
Right ascension00 35 23.1
Declination−23° 22′ 30″
Redshift0.012812
Distance172 Mly
Apparent magnitude (V)13.98
Characteristics
TypeSbc
Apparent size (V)1.0' × 0.7'
Other designations
PGC 2122

NGC 167 is a spiral galaxy located approximately 172 million light-years from the Solar System in the constellation Cetus. It was discovered in 1886 by Francis Preserved Leavenworth.

See also

References

  1. ^ "NASA/IPAC Extragalactic Database". Results for NGC 0167. Retrieved 2016-09-02.
  2. ^ An object's distance from Earth can be determined using Hubble's law: v=Ho is Hubble's constant (70±5 (km/s)/Mpc). The relative uncertainty Δd/d divided by the distance is equal to the sum of the relative uncertainties of the velocity and v=Ho
  3. "NGC 167". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 12 February 2017.
  4. "New General Catalog Objects: NGC 150 - 199". cseligman.com. Retrieved 12 February 2017.

External links


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