This system is located at:
R: 17,929.994 / l: 29.712 / b: -0.240
Right ascension: 18h 46m 24.955s / Declination: -2° 58'30.069''
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)
This system was visited for the first time on EDSM by Irisa Nyira on Jul 6, 2016, 9:42:32 AM.
It was named by the Galactic Mapping Project with the name of: The Kes-75 Magnetar
211 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.