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词条 NGC 227
释义

  1. See also

  2. References

  3. External links

{{Infobox galaxy
| name = NGC 227
| image = NGC227 - SDSS DR14.jpg
| caption = SDSS image of NGC 227
| epoch = J2000
| ra = {{RA|00|42|36.8}}[1]
| dec = {{DEC|-01|31|44}}[1]
| constellation name = Cetus
| z = 0.017669[1]
| dist_ly =237 Mly[2]
| type = S0[1]
| appmag_v = 13.11[1]
| size_v = 1.6' × 1.3'[1]
| notes =
| names = UGC 456, CGCG 383-076, MCG +00-02-135, 2MASX J00423684-0131436, 2MASXi J0042365-013137, 6dF J0042367-013144, PGC 2547.[1]
}}NGC 227 is a lenticular galaxy located approximately 237 million light-years from the Sun[2] in the constellation Cetus. It was discovered on October 1, 1785 by William Herschel.[3]

See also

  • Lenticular galaxy
  • List of NGC objects (1–1000)
  • Cetus

References

1. ^{{cite web | title=NASA/IPAC Extragalactic Database | work=Results for NGC 0227 | url=http://ned.ipac.caltech.edu/cgi-bin/objsearch?objname=NGC+227&extend=no&hconst=73&omegam=0.27&omegav=0.73&corr_z=1&out_csys=Equatorial&out_equinox=J2000.0&obj_sort=RA+or+Longitude&of=pre_text&zv_breaker=30000.0&list_limit=5&img_stamp=YES | accessdate=2016-09-02}}
2. ^An object's distance from Earth can be determinded 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. ^{{cite web|title=New General Catalog Objects: NGC 200 - 249|url=http://cseligman.com/text/atlas/ngc2.htm#227|publisher=Cseligman|accessdate=September 15, 2016}}

External links

  • {{WikiSky}}
  • SEDS
{{Ngc5}}{{Catalogs|PGC=2547|UGC=456|NGC=227}}{{Sky|00|42|36.8||-01|31|44|190000000}}

6 : NGC objects|Principal Galaxies Catalogue objects|Lenticular galaxies|Cetus (constellation)|Astronomical objects discovered in 1785|Discoveries by William Herschel

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