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Messier 52: Difference between revisions
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Messier 52 (also known as M 52 or NGC 7654) is an open cluster in the [[Cassiopeia]] constellation. It was discovered by Charles Messier in 1774. M52 can be seen from Earth with binoculars.Due to interstellar absorption of light, the distance to M 52 is uncertain, with estimates ranging between 3,000 and 7,000 light years. One study identified 193 probable members of the cluster, with the brightest member being magnitude 11. | Messier 52 (also known as M 52 or NGC 7654) is an open cluster in the [[Cassiopeia]] constellation. It was discovered by Charles Messier in 1774. M52 can be seen from Earth with binoculars.Due to interstellar absorption of light, the distance to M 52 is uncertain, with estimates ranging between 3,000 and 7,000 light years. One study identified 193 probable members of the cluster, with the brightest member being magnitude 11. | ||
Messier 52 is evaluated at about 35 million years old. <ref>[http://en.wikipedia.org/wiki/Messier_52 Messier 52]</ref> | Messier 52 is evaluated at about 35 million years old. <ref>[http://en.wikipedia.org/wiki/Messier_52 Messier 52]</ref> | ||
==Session References== | ==Session References== | ||
HGS Sessions - [[Clearing Nibiru Nets]] - 3/11/2015 <ref>HGS Session</ref>HGS Sessions - Clearing [[Temple Mount, Jerusalem.]] - 3/20/2015 <ref>HGS Session</ref> HGS Sessions - Clearing [[Dorado, Leo Minor, Musca, Perseus constellations]] - 3/23/2015 <ref> HGS Session</ref> | HGS Sessions - [[Clearing Nibiru Nets]] - 3/11/2015 <ref>HGS Session</ref>HGS Sessions - Clearing [[Temple Mount, Jerusalem.]] - 3/20/2015 <ref>HGS Session</ref> HGS Sessions - Clearing [[Dorado, Leo Minor, Musca, Perseus constellations]] - 3/23/2015 <ref> HGS Session</ref> | ||
==References== | ==References== | ||
<references/> | <references/> | ||
Found in HGS Manual on Page 108 | |||
Found in HGS Manual on Page | Found in HGS Manual on Page 115 | ||
[[Category: Ascension]][[Category: HGS Manual]] | [[Category: Ascension]][[Category: HGS Manual]] | ||