Celestial hemisphere:  Southern  ·  Constellation: Capricornus (Cap)
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The Ptolemy's Cluster (Messier 7), Leo Pires
The Ptolemy's Cluster (Messier 7)
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The Ptolemy's Cluster (Messier 7)

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The Ptolemy's Cluster (Messier 7), Leo Pires
The Ptolemy's Cluster (Messier 7)
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The Ptolemy's Cluster (Messier 7)

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Description

=_aacl _aaco _aacu _aacx _aad7 _aadeThis is a bright open cluster in Scorpius constellation. The cluster lies at an approximate distance of 980 light years from Earth and it's an easy naked-eye target.

M7 is one of the most prominent open clusters in the sky, known since antiquity. It was named Ptolemy’s Cluster because it was first recorded by the Greek astronomer and mathematician Claudius Ptolemy in the 2nd century. Ptolemy listed the cluster in his Almagest as Object Number 567 and described it as a “nebula following the sting of Scorpius” in 130 AD.

Italian astronomer Giovanni Batista Hodierna counted 30 stars in the cluster before 1654. In 1678, English astronomer Edmond Halley included the cluster in his catalogue of southern stars as No. 29.

French astronomer Nicolas Louis de Lacaille observed the cluster on June 15, 1752 and listed it as Lac. II.14 in his catalogue of southern objects. He described the cluster as a “group of 15 or 20 stars very close together, in the figure of a square.”

Charles Messier included the cluster as the seventh entry in his catalogue on May 23, 1764. He described it as a “star cluster, more considerable than the preceding [Messier 6]; to the naked eye, this cluster looks like a nebulosity; it is little distant from the preceding, placed between the bow of Sagittarius & the tail of Scorpius.”

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The Ptolemy's Cluster (Messier 7), Leo Pires