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> | |||
==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]] | ||
Latest revision as of 21:37, 23 March 2015
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. [1]
Session References
HGS Sessions - Clearing Nibiru Nets - 3/11/2015 [2]HGS Sessions - Clearing Temple Mount, Jerusalem. - 3/20/2015 [3] HGS Sessions - Clearing Dorado, Leo Minor, Musca, Perseus constellations - 3/23/2015 [4]
References
- ↑ Messier 52
- ↑ HGS Session
- ↑ HGS Session
- ↑ HGS Session
Found in HGS Manual on Page 108
Found in HGS Manual on Page 115