NGC 342 | |
---|---|
![]() SDSS image of NGC 342 | |
Observation data (J2000 epoch) | |
Constellation | Cetus |
Right ascension | 01h 00m 49.8s[1] |
Declination | −06° 46′ 21″[1] |
Redshift | 0.019403[1] |
Heliocentric radial velocity | 5,817 km/s[1] |
Apparent magnitude (V) | 15.41[1] |
Characteristics | |
Type | S0 |
Apparent size (V) | 0.6' × 0.3'[1] |
Other designations | |
MCG -01-03-058, 2MASX J01004985-0646207, 2MASXi J0100498-064620, 6dF J0100499-064621, PGC 3631.[1] |
NGC 342 is a lenticular galaxy in the constellation Cetus. It was discovered on September 27, 1864 by Albert Marth. It was described by Dreyer as "very faint, very small."[2]
References
[edit]- ^ a b c d e f g "NASA/IPAC Extragalactic Database". Results for NGC 0342. Retrieved September 2, 2016.
- ^ "New General Catalog Objects: NGC 300 - 349". Cseligman. Retrieved November 6, 2016.
External links
[edit]Media related to NGC 342 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