V4641 Sagittarii [#689407301]
This system is located at:
R: 29,999.996 / l: 6.774 / b: -4.789
Right ascension: 18h 19m 21.651s / Declination: -25° 24'25.748''
Metal-rich body (27 to 930 ls), Earth-like world (14,642 to 21,960 ls), Water world (12,006 to 46,497 ls), Ammonia world (30,378 to 82,662 ls), Terraformable (11,404 to 22,754 ls)
This system was visited for the first time on EDSM by Squirts MacIntosh on May 14, 2016, 6:38:52 PM.
33 ships passed through V4641 Sagittarii space, including 0 ship in the last 7 days.
0 ship passed through V4641 Sagittarii space in the last 24 hours.
V4641 Sagittarii is a variable X-ray binary star system in the constellation Sagittarius. It is the source of one of the fastest superluminal jets in the Milky Way galaxy. Amateur astronomer Rod Stubbings made a visual observation of a dramatic outburst during earth year 1999. This observation helped to confirm the source was a black hole with a close binary star.
Survey in 3303 confirmed the black hole of 7 sol masses was closely orbited by a class-A super-giant of 7 solar masses and 11.7 solar radius. The extreme x-ray bursts and jets are caused by matter in-falling to the black hole from the surface of the supergiant.