Messier 95: Difference between revisions
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HGS Sessions - Clearing [[Planet Verticals]] - 3/17/2015 <ref>[http://www.energeticsynthesis.com/index.php/forum/52-hgs-discussions-and-q-a-a/60650-hgs-shared-sessions-and-discussion?start=126h HGS Session]</ref> | HGS Sessions - Clearing [[Planet Verticals]] - 3/17/2015 <ref>[http://www.energeticsynthesis.com/index.php/forum/52-hgs-discussions-and-q-a-a/60650-hgs-shared-sessions-and-discussion?start=126h HGS Session]</ref> | ||
HGS Sessions - Clearing [[Temple Mount, Jerusalem.]] - 3/20/2015 <ref>[http://www.energeticsynthesis.com/index.php/forum/planetary-emancipation-gridwork-peg/60919-documenting-hgs-sessions-for-peg-gridwork?start=48#101346 HGS Session]</ref> | |||
==References== | ==References== | ||
Latest revision as of 23:07, 20 March 2015
Messier 95 (also known as M95 or NGC 3351) is a barred spiral galaxy about 38 million light-years away in the constellation Leo. It was discovered by Pierre Méchain in 1781, and catalogued by Charles Messier four days later. On 16 March 2012, a supernova was discovered in M95.
M95 is one of several galaxies within the M96 Group, a group of galaxies in the constellation Leo. The group also includes the Messier objects Messier 96 and Messier 105.
HGS Session References
HGS Sessions - Clearing Planet Verticals - 3/17/2015 [1] HGS Sessions - Clearing Temple Mount, Jerusalem. - 3/20/2015 [2]
References
Found in HGS Manual on Page 108
Found in HGS Manual on Page 115