Messier 7
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Messier 7 or M7, also designated NGC 6475 and sometimes known as Ptolemy's Cluster,<ref name=gendler2011/><ref name=Ridpath/> is an open cluster of stars in the constellation of Scorpius. The cluster is easily detectable with the naked eye, close to the "stinger" of Scorpius. With a declination of −34.8°, it is the southernmost Messier object.
Observations
M7 has been known since antiquity; it was first recorded by the 2nd-century Greek-Roman astronomer Ptolemy, who described it as a nebula in 130 AD.<ref name=jones1991/> Italian astronomer Giovanni Batista Hodierna observed it before 1654 and counted 30 stars in it. In 1764, French astronomer Charles Messier catalogued the cluster as the seventh member in his list of comet-like objects. English astronomer John Herschel described it as "coarsely scattered clusters of stars".<ref name=gendler2011/> In Chinese astronomy it is identified as Yú, the Fish (Template:Lang-zh).<ref name=Ridpath/><ref name=AEEA/>
Telescopic observations of the cluster reveal about 80 stars within a field of view of 1.3° across. At the cluster's estimated distance of 980 light years this corresponds to an actual diameter of 25 light years. The tidal radius of the cluster is Template:Convert and it has a combined mass of about 735 times the mass of the Sun.<ref name=aaa477_1_165/> The age of the cluster is around 200<ref name=aaa504_3_845/> million years while the brightest member star is of magnitude 5.6. In terms of composition, the cluster contains a similar abundance of elements other than hydrogen and helium as the Sun.<ref name=aaa504_3_845/>
On August 29, 2006, Messier 7 was used for first light image of the Long Range Reconnaissance Imager (LORRI) telescope on the Pluto-bound New Horizons spacecraft.<ref>Template:Cite web</ref>
As of January 2022, Messier 7 is one of the few remaining Messier objects not photographed by the Hubble Space Telescope.<ref>Template:Cite web</ref> This is mainly due to those objects' angular diameter or lack of scientific significance. Most such objects are open clusters of large angular diameter that would require thousands of photos due to Hubble's small field of view. (For comparison, Hubble's well known panoramic photo of the Andromeda Galaxy, covering less than half of our galactic neighbor, required approximately 400 individual movements and 7400 exposures.)<ref>Template:Cite web</ref>
Brightest members
Messier 7 contains over a thousand likely members stars spread across several degrees. Member's brighter than about 8th magnitude have evolved away from the main sequence, with the most luminous main sequence stars around spectral class A0. The brightest stars with a membership probability higher than 75%:<ref name=cg2020>Template:Cite journal</ref>
Gallery
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M7 on the night sky. It is easily visible to the naked eye and located between the constellations Scorpius and Sagittarius.
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Broader view of M7, with the cluster at the center of the image
See also
References
External links
- Messier 7, SEDS Messier pagesTemplate:WikiSky
- Template:APOD
- New Horizons probe captures M7
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