Template:Short description Template:Galaxy cluster Seyfert's Sextet is a group of galaxies about 190 million light-years away<ref>{{#invoke:citation/CS1|citation |CitationClass=web }} </ref> in the constellation Serpens. The group appears to contain six members, but one of the galaxies, NGC 6027d, is a background object (700 million light years behind the group) and another "galaxy," NGC 6027e, is actually a part of the tail from galaxy NGC 6027. The gravitational interaction among these galaxies should continue for hundreds of millions of years. Ultimately, the galaxies will merge to form a single giant elliptical galaxy.

DiscoveryEdit

French astronomer Édouard Stephan discovered NGC 6027 on 20 March 1882, but he was unable to resolve the individual galaxies in the group.<ref name="selig">{{#invoke:citation/CS1|citation |CitationClass=web }}</ref> The group members were discovered by Carl Keenan Seyfert using photographic plates made at the Barnard Observatory of Vanderbilt University. When these results were first published in 1951, this group was the most compact group ever identified.<ref name="bajajaetal1984">Template:Cite journal</ref>

MembersEdit

Members of Seyfert's Sextet
Name Type Distance from Sun
(million ly)
Magnitude
NGC 6027 S0 pec. ~190 +14.7
NGC 6027a Sa pec. ~190 +15.4
NGC 6027b S0 pec. ~190 +15.4
NGC 6027c SB(S)c ~190 +16
NGC 6027d SB(S)bc pec. citation CitationClass=web

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+15.6
NGC 6027e Tidal Tail. ~190 +16.5

See alsoEdit

ReferencesEdit

Template:Reflist

External linksEdit

Template:Sky Template:Serpens