PHEIA AUSCS XU-X D1-355 is a seemingly dull, unremarkable system which, at first glance, doesn't offer much for the intrepid explorer. However, while cruising in system if one turns the right way they will be greeted with a splendid view of the nearby nebula surrounding the PHEIA AUSCS V0-A E20 system, which houses a neutron star and several bodies.

PHEIA AUSCS XU-X D1-355 itself offers a single landable planet in BC 3 A, however, which may stun the CMDR who steps out of his ship onto the surface, as that nearby nebula now fills the sky like the exploding remnant of a massive, ancient, stellar phoenix.

The twin Class M stars, which form the barycenter that all the planetary bodies of the system orbit, hover just outside the view of the nebula, as though they were a pair of twin phoenix eggs left behind from the fiery death of the parent. Some CMDRs consider it a promise, as though the fiery remnants represent a sort of crucible for new life, light, and warmth.

While it isn't certain that the nebula in question was actually involved in the formation of the two Class M stars of this system, the rather romantic notion has resulted in earning the stars and nebula as viewed from BC 3 A the nickname "Phoenix Twins."

PHEIA AUSCS XU-X D1-355 is a seemingly dull, unremarkable system which, at first glance, doesn't offer much for the intrepid explorer. However, while cruising in system if one turns the right way they will be greeted with a splendid view of the nearby nebula surrounding the PHEIA AUSCS V0-A E20 system, which houses a neutron star and several bodies.

PHEIA AUSCS XU-X D1-355 itself offers a single landable planet in BC 3 A, however, which may stun the CMDR who steps out of his ship onto the surface, as that nearby nebula now fills the sky like the exploding remnant of a massive, ancient, stellar phoenix.

The twin Class M stars, which form the barycenter that all the planetary bodies of the system orbit, hover just outside the view of the nebula, as though they were a pair of twin phoenix eggs left behind from the fiery death of the parent. Some CMDRs consider it a promise, as though the fiery remnants represent a sort of crucible for new life, light, and warmth.

While it isn't certain that the nebula in question was actually involved in the formation of the two Class M stars of this system, the rather romantic notion has resulted in earning the stars and nebula as viewed from BC 3 A the nickname "Phoenix Twins."