 Artist impression of a gamma-ray burst | |
| Event type | Gamma-ray burst |
|---|---|
| Date | c. 3 billion years ago (detected 9 May 2005) |
| Instrument | Swift |
| Constellation | Coma Berenices |
| Right ascension | 12h 36m 13.9s |
| Declination | +28° 59′ 01″ |
| Distance | c. 3 billion ly |
| Redshift | 0.225 |
| Other designations | GRB 050509B |
GRB 050509B was a gamma-ray burst (GRB) observed by the NASA Swift satellite on May 9, 2005. It was the first short duration GRB for which an accurate positional measurement was made, accurate enough to locate it near to an elliptical galaxy lying at a redshift of 0.225.
The significance of this finding is that it lends support to the theory that short bursts are formed during the catastrophic merger of two neutron stars, or a neutron star and a black hole. The orbital decay (via gravitational radiation) of stellar binaries consisting of these exotic compact objects is believed to take hundreds of millions of years, hence gamma ray bursts produced this way would be expected to be in old (misleadingly called "early type") galaxies. In contrast, long-duration gamma ray bursts, which are believed to result from the collapse of a single massive star, are expected to be located preferentially in young galaxies.
References[edit]
- David Whitehouse (11 May 2005). "Blast hints at black hole birth". BBC News. Retrieved 12 July 2011.
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