NGC 1545 explained

NGC 1545
Type:Open Cluster
Epoch:J2000
Constellation:Perseus
Ra:[1]
Dist Ly:2,320 ly
Dist Pc:711 pc[2]
Appmag V:6.4
Size V:23'
Age:280 millions years
Names:Cr 49

NGC 1545 is an open cluster in the constellation Perseus. It was discovered by William Herschel on December 28, 1790.[3] It is located in the north-eastern part of the constellation, a few arcminutes east of the 4.5 magnitude star b Persei, near the equally large and bright NGC 1528 (m = 6.4), which is less than 1.5° towards the northwest. However, it is less dense and rich. The brightest star of the cluster is a K5 III giant star, with 7.1 magnitude, but its membership is questionable. One more 7.9 magnitude star is visible at the north edge of the cluster.[4]

Notes and References

  1. Web site: SIMBAD Astronomical Database. Results for NGC 1545. 2015-06-19.
  2. http://www.univie.ac.at/webda/cgi-bin/ocl_page.cgi?dirname=ngc1545 WEBDA: NGC 1545
  3. Web site: Seligman . Courtney . NGC 1545 (= OCL 399 = "PGC 3518640") . Celestial Atlas . 7 December 2018.
  4. Book: Craig Crossen. Gerald Rhemann. amp. Sky Vistas: Astronomy for Binoculars and Richest-Field Telescopes. 2012. Springer Science & Business Media. 9783709106266. 95. 30 October 2015.