NGC 6603 explained

NGC 6603
Constellation:Sagittarius
Epoch:J2000.0
Class:I,2,r,n
Ra:18h 18.4m
Dec:-18° 25
Dist Ly:10 kly
Appmag V:11.1 [1]
Size V:5
Names:Collinder 374

NGC 6603 is an open cluster discovered by John Herschel on July 15, 1830[2] located in Sagittarius constellation.[3]

Situated within the brightest part of star cloud Messier 24, it is classified by Shapley as type "g". This cluster consists of about 30 stars in a field of about 5 arc minutes in diameter, and is about 9400 light years remote. Thus its linear diameter should be about 14 light years. The hottest stars are about B9 (pointing to an intermediate age of several 100 million years, an estimate of which is not known to the present author), and the brightest of photographic mag 14.

Many sources improperly identify NGC 6603 as Messier 24.[4]

Notes and References

  1. Web site: ngc 6603. 2020-06-10. sim-id.
  2. Web site: Seligman. Courtney. Celestial Atlas: NGC Objects 6600-6649. cseligman.com. 2 July 2015. https://web.archive.org/web/20150909235453/http://cseligman.com/text/atlas/ngc66.htm. 9 September 2015. dead.
  3. Web site: Open cluster NGC 6603 - Open Cluster in Sagittarius Constellation. Rojas. Sebastián García. Telescopius. en. 2019-12-26.
  4. Web site: Messier 24. messier.seds.org. en-US. 2020-09-27. 2023-04-16. https://web.archive.org/web/20230416102130/https://www.messier.seds.org/m/m024.html. dead.