PSR J1846-0258 (The Kes-75 Magnetar) [#134738909]
This system is located at:
-8886.75
/ -75.15625
/ 15572.5625
Galaktické souřadnice
R: 17 929,994 / l: 29,712 / b: -0,240
Rovníkové koordináty:
Stoupání 18h 46m 24,955s /
Deklinace: -2° 58'30,069''
Reserve level: Nedotčené
Obyvatelná zóna:
Metal-rich body (0 to 3 688 508 ls), Earth-like world (58 064 690 to 87 086 330 ls), Water world (47 612 935 to 184 396 428 ls), Ammonia world (120 472 267 to 327 815 872 ls), Terraformable (45 225 210 to 90 238 522 ls)
Předpokládaná hodnota: 131 911 CR
This system was visited for the first time on EDSM by Irisa Nyira on 6. 7. 2016 9:42:32.
It was named by the Galactic Mapping Project with the name of: The Kes-75 Magnetar
206 ships passed through PSR J1846-0258 space, including 0 ship in the last 7 days.
0 ship passed through PSR J1846-0258 space in the last 24 hours.
Also known as PSR J1846-0258, this is a 14.07 solar mass pulsar at the center of supernova remnant Kes-75. This pulsar is believed to be of a subcategory called a magnetar, having extremely powerful magnetic fields which cause powerful radiation bursts. They are widely believed to be the source of the so-called 'soft gamma repeater' (SGR), an astronomical object which emits large bursts of gamma-rays and X-rays at irregular intervals. PSR J1846-0258 is a 326-ms pulsar; it emits roughly three pulses per second.
The magnetar shares a binary orbit with another neutron star of 1.3 solar masses, and an F-type star. Several sub-stellar dwarves (Y, L, T) and smaller bodies are also present.
Thanks is given to Cmdr Kazahnn for helping to update this entry.
