NGC 767 | |
---|---|
![]() SDSS image of NGC 767 | |
Observation data (J2000 epoch) | |
Constellation | Cetus |
Right ascension | 01h 58m 50.822s |
Declination | −09° 35′ 13.61″ |
Redshift | 0.01805[1] |
Heliocentric radial velocity | 5362 km/s[1] |
Distance | 246.5 ± 17.3 Mly (75.58 ± 5.3 Mpc)[2] |
Apparent magnitude (B) | 14[1] |
Characteristics | |
Type | SBb pec?[2] |
Other designations | |
PGC 7483[1] |
NGC 767 is a barred spiral galaxy located in the constellation Cetus about 241 million light years from the Milky Way. It was discovered by the American astronomer Francis Leavenworth in 1886.[3][4][5]
See also
[edit]References
[edit]- ^ a b c d "NGC 767". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2020-05-24.
- ^ a b "Results for object NGC 0767 (NGC 767)". NASA/IPAC Extragalactic Database. California Institute of Technology. Retrieved 2020-05-24.
- ^ "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2020-03-30.
- ^ "Revised NGC Data for NGC 767". spider.seds.org. Retrieved 2020-03-30.
- ^ Ford, Dominic. "The galaxy NGC 767 - In-The-Sky.org". in-the-sky.org. Retrieved 2020-03-30.
External links
[edit]Media related to NGC 767 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