Vela Pulsar [#27105682612]
This system is located at:
905.9375
/ -44.40625
/ -102.40625
Galaktické souřadnice
R: 912,788 / l: 263,551 / b: -2,788
Rovníkové koordináty:
Stoupání 8h 35m 20,066s /
Deklinace: -45° 10'34,220''
Obyvatelná zóna:
Metal-rich body (0 to 1 658 760 ls), Earth-like world (26 112 291 to 39 163 622 ls), Water world (21 412 028 to 82 924 978 ls), Ammonia world (54 177 623 to 147 422 183 ls), Terraformable (20 338 244 to 40 581 195 ls)
Předpokládaná hodnota: 48 947 CR
This system was visited for the first time on EDSM by Guy De Lombard on 22. 7. 2015 15:30:51.
1381 ships passed through Vela Pulsar space, including 3 ships in the last 7 days.
0 ship passed through Vela Pulsar space in the last 24 hours.
The Vela Pulsar is a radio, optical, X-ray- and gamma-emitting pulsar associated with the Vela Supernova Remnant in the constellation of Vela. The spin of 11.195 times per second (i.e. a period of 89.33 milliseconds) was the shortest known at the time of discovery.
The pulsar was discovered by astronomers at the University of Sydney in 1968, and was the direct evidence that supernovae form neutron stars. It was also studied in 2015 by a NASA balloon launched from Alice Springs, Australia. Perhaps most unusually, the emissions of Vela and the pulsar PSR B0329+54 were converted into audible sound by French composer Gérard Grisey and used in the piece 'Le noir de l'étoile'.
The Vela Pulsar is in binary pair with a B-class star and also is found with a number of class V gas giants.
