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{{Galaxy cluster
| name = Abell 569
| image =
| epoch = J2000
| constellation = Lynx
| ra = {{RA|07|09|10.4}}
| dec = {{DEC|+48|37|10}}
| member_no =
| brightest_member =
| richness =
| bmtype = II
| velocity_dispersion = 500[1]
| redshift = 0.019417[1]
| distance =
| temperature =
| mass =
| luminosity =
| flux =
| other_names = A 569
}}Abell 569 is a galaxy cluster in the northern constellation of Lynx. It is organized into two primary condensations that are separated by about 1.5 Mpc, and is probably a member of the Perseus Supercluster. The brightest galaxy in the cluster is NGC 2329, a giant elliptical galaxy of type D that is associated with a radio and X-ray source.References1. ^1 2 {{citation | display-authors=1 | last1=Hudson | first1=Michael J. | last2=Lucey | first2=John R. | last3=Smith | first3=Russell J. | last4=Schlegel | first4=David J. | last5=Davies | first5=Roger L. | title=Streaming motions of galaxy clusters within 12 000 km s-1 - III. A standardized catalogue of Fundamental Plane data | journal=Monthly Notices of the Royal Astronomical Society | volume=327 | issue=1 | pages=265–295 | date=October 2001 | doi=10.1046/j.1365-8711.2001.04786.x | bibcode=2001MNRAS.327..265H | postscript=. }}
}}{{Catalogs|Abell=569}}{{galaxy}} 3 : Lynx (constellation)|Abell objects|Galaxy clusters |