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Ptolomey’s Cluster, M7 (NGC 6475, The Scorpion’s Tail), Paul Lloyd
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Ptolomey’s Cluster, M7 (NGC 6475, The Scorpion’s Tail)

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Description

Ptolemy, the Greek-Roman mathematician and astronomer, recorded this object in his famous
Almagest as entry #567 in 130CE. One has to admire this as this open star cluster rises only
a short distance above his horizon in mid-Summer, and he had no optical aid. He described it
as a “nebula following the sting of Scorpius”.

It can be seen with the naked eye just North of the Scorpion’s “stinger”. It comprises some 80
stars with magnitudes between 6 and 10. These are mainly white/blue-white in colour, with
one exception (lower SW corner) being a yellow G8-class star. It is approx. 25 ly in diameter,
and lies 980 ly away. It is one of the most prominent open clusters in the sky, and is the most
southerly Messier object. It is believed to be about 220 Myo and has a mass about 735 times
that of the Sun. It is currently approaching us.


Telescope: William Optics Redcat71 refractor, f=350mm
Camera:     ZWO ASI183MC Pro, 60 x 120 sec, no filter
                   Bortle 3-4 sky, moonless (before moonrise)
Field of View: approx. 1º 00’ x 1º 25’
Image processed and prepared in PixInsight and Photoshop Elements

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Ptolomey’s Cluster, M7 (NGC 6475, The Scorpion’s Tail), Paul Lloyd