| NGC 1027 | |
|---|---|
 NGC 1027 (taken from Stellarium) | |
| Observation data (J2000 epoch) | |
| 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] |
| Other designations | Cr 30 |
| Associations | |
| Constellation | Cassiopeia |
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 a member of the cluster. The brightest member of the cluster has an apparent magnitude of 9,3.[3]
References[edit]
- ^ a b c "NGC 1027". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2015-06-19.
- ^ a b 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 978-3-7091-0626-6.
External links[edit]
Media related to NGC 1027 at Wikimedia Commons
Well, that’s interesting to know that Psilotum nudum are known as whisk ferns. Psilotum nudum is the commoner species of the two. While the P. flaccidum is a rare species and is found in the tropical islands. Both the species are usually epiphytic in habit and grow upon tree ferns. These species may also be terrestrial and grow in humus or in the crevices of the rocks.
View the detailed Guide of Psilotum nudum: Detailed Study Of Psilotum Nudum (Whisk Fern), Classification, Anatomy, Reproduction