NGC 2455 Open Cluster in Puppis
I used telescope T9 at Siding Spring to image this open cluster using V and B Filters. Telescope T9 is regularly used in Hubble Space Telescope support missions. This cluster was discovered on 15th February 1836 by John Herschel, the son of William Herschel. The stars are generally around 12th Magnitude. The cluster is approximately 5' across. The field of view of telescope T9 is 13.6 x 20.4 arc-mins. The cluster lies at a distance of 2650 Parsecs. (Ref 1) The bright foreground star is HIP 38197 with a magnitude of V =7.95 and B = 7.80 so is slightly brighter in the blue. It lies at a distance of 1,716 Light Years which is 526 Parsecs so it lies at about one fifth of the distance of the cluster from us.
The chart below shows the position of NGC 2455 in Puppis.(Courtesy of Ref 2)