NGC 6242 explained

NGC 6242
Credit:DECaPS
Appmag V:6.4
Age:77.6 Myr

NGC 6242 is an open cluster of stars in the southern constellation Scorpius. It can be viewed with binoculars or a telescope at about 1.5° to the south-southeast of the double star Mu Scorpii. This cluster was discovered by French astronomer Nicolas-Louis de Lacaille in 1752 from South Africa. It is located at a distance of approximately from the Sun, just to the north of the Sco OB 1 association. The cluster has an estimated age of 77.6 million years.

A microquasar with the designation GRO J1655-40 is located in the vicinity of NGC 6242 and is moving away from the cluster with a runaway space velocity of . It may have originated in the cluster during a supernova explosion ago.

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