Pha Scroi GS-I d10-64 (Minerva's Pyrope) [#2207521362651]
This system is located at:
-9453.84375
/ 2207.25
/ 24186.96875
Galactic coordinates:
R: 26 062,551 / l: 21,349 / b: 4,858
Equatorial coordinates:
Right ascension: 18h 12m 41,685s /
Declination: −8° 0'55,727''
Habitable zone:
Metal-rich body (67 to 207 ls), Earth-like world (3 266 to 4 899 ls), Water world (2 678 to 10 372 ls), Ammonia world (6 777 to 18 440 ls), Terraformable (2 544 to 5 076 ls)
Estimated value: 554 425 cr
This system was visited for the first time on EDSM by Rory Clague.
It was named by the Galactic Mapping Project with the name of: Minerva's Pyrope
22 ships passed through Pha Scroi GS-I d10-64 space, including 0 ship in the last 7 days.
0 ship passed through Pha Scroi GS-I d10-64 space in the last 24 hours.
This J-type carbon star (rich in diatomic carbon and cyanogen containing carbon-13) was discovered in the final weeks of the Minerva-Centaurus Expedition. C-J stars are among the rarest stars in the galaxy, constituting only 10-15% of all carbon stars. They are typically dimmer than N-type carbon stars, and this particular specimen is among the coldest (2703 K) and least luminous (0.7569) C-J stars in the galaxy and at the time of its discovery held the records for these parameters. The star's dimness combined with its carbon-rich corona have created a sooty red glow visible around the system, illuminating an ancient Earth-like world. The presence of an Earth-like world in this environment would be of special interest to astrobiologists interested in the carbon-13 enriched biochemistry of the native flora and fauna. The immense age of the system (12.937 Ga) may also be of interest to researchers studying the evolution of Earth-like planets late in the life of stars with near-solar masses (0.92). The presence of an ELW in this rare star type is certainly a welcome surprise to travellers in the Far 3kpc Arm.
Evidence of uniqueness/significance: Faintest C-J star, Coldest C-J star, Record as of 18 March 2018, Contains an Earth-like world.
Reference : LINK