NGC 1027
| NGC 1027 | |
|---|---|
 NGC 1027 (taken from Stellarium) | |
| Observation data (J2000 epoch) | |
| Constellation | Cassiopeia |
| Right ascension | 02h 42m 43s[1] |
| Declination | +61° 38′ 00″[1] |
| Distance | 3,100 ly (950 pc[2]) |
| Apparent magnitude (V) | 6.7 [1] |
| Apparent dimensions (V) | 20' |
| Physical characteristics | |
| Estimated age | 355 millions years [2] |
NGC 1027 is an open cluster in the constellation Cassiopeia. It was discovered by William Herschel in 1787. It is visible at the eastern part of the constellation, between two emission nebulae, the Heart and Soul Nebula. However, it is not physically associated with the two nebulae, lying in the foreground, about 3,000 light years away from the Solar System. The apparent magnitude of the cluster is 6.7 and can be seen with 10x50 binoculars around a 7th magnitude star, which is not however member of the cluster. The brightest member of the cluster has apparent magnitude 9,3.[3]
References
- 1 2 3 "SIMBAD Astronomical Database". Results for NGC 1027. Retrieved 2015-06-19.
- 1 2 Global survey of star clusters in the Milky Way. II. The catalogue of basic parameters.
- ↑ Craig Crossen & Gerald Rhemann (2012). Sky Vistas: Astronomy for Binoculars and Richest-Field Telescopes. Springer Science & Business Media. p. 87. ISBN 9783709106266. Retrieved 30 October 2015.
This article is issued from Wikipedia - version of the 5/9/2016. The text is available under the Creative Commons Attribution/Share Alike but additional terms may apply for the media files.