35 Gamma Cephei

35 Gamma Cephei
 * UAS: Errai 
 * Union system
 * stellar class K1III-IV orange subgiant star
 * M-0 Galaxy, Upward Sector

Single planet (Supergiant), substantial asteroid belt.

The system is about 45 Light years from Sol and is located  within the main traffic corridor to Blue Moon. It was an important logistics and fuel stop system before the Space Train and the HHW came on line.

It has been surveyed by United Earth around 2200 OTT and the first colonists ( the moons around Cephei, planet ) and the asteroid belt) were mostly miners and resource gatherers.

A large space space station was placed in an apex position over the main star early on.

The system has somewhat lost its importance after faster and direct traffic connections to Blue Moon became available. But it is still home to over 6 billion. Asteroid mining and fuel production are still core industries.

But the character is slowly changing as more and more asteroids are used for large private residence objects. The system still has a Class A spaceport and a Space Train connection to both Sol and Blue Moon.

Pre Astro System Info
Gamma Cephei (γ Cep, γ Cephei), traditionally named Errai, Er Rai, and or Alrai, is a binary star system approximately 45 light-years away in the constellation of Cepheus. Gamma Cephei contains an apparent magnitude of 3.22. The visible part of the system is a stellar class K1III-IV orange subgiant star on its first ascent off the main sequence. It is about 6.6 billion years old (based on Fe/H metallicity).[4] Since 1943, the spectrum of this star has served as one of the stable anchor points by which other stars are classified.[5]

Gamma Cephei is the naked-eye star that will succeed Polaris as the Earth's northern pole star, due to the precession of the equinoxes. It will be closer to the northern celestial pole than Polaris around 3000 CE and will make its closest approach around 4000 CE. The "title" will pass to ι Cephei some time around 5200 CE.

The star has a companion star with a mass approximately 0.409 times that of our Sun.[2] Gamma Cephei B is of stellar mass and is assumed to be of similar age to its primary. It is probably a red dwarf of class M4, 6.2 degrees of magnitude fainter than the K-type primary star.[2]