Mirri System

The Mirri System is a star system within the Orion Arm of the Milkyway Galaxy. Mirri is a M-type main-sequence Red Dwarf with seven planets: five terrestrial and two gas giants. Mirri is quite difficult for outside exploration due to the star’s low luminosity and age, the system is cold and dimly lit. Needless to say, the Asiel, Mirri's native near-human humanoid race, have adapted to these conditions due to their highly advanced technology.

Age 10.3 billion years

Galaxy Milky Way

Galactic Arm Orion

Distance from Sol 785 light-years

Nearest star(s)

Almesi (Approx. 3.89 light-years)

Titire (Approx. 4.25 light-years)

Varg (Approx. 4.72 light-years)

Native Race

Asiel (homeworld: Airinia)

Population

Stars Mirri

Planets

• Mirri I (0.103 AU)

• Mirri II (0.164 AU)

• Mirri III (0.173 AU)

• Mirri IV (Airinia; 0.182 AU)

• Mirri V (5 AU)

• Mirri VI (5.847 AU)

• Mirri VII (7.483 AU)

Known dwarf planets 16

Known natural satellites 216

Known minor planets 23

Known comets 3,624

Planetary system

Star spectral type M4 V

Frost line ~2.97AU

Semi-major axis of the Outermost planet 7.483 AU

Heliopause detected at 89.2 AU

Hill sphere 0.42 parsecs (~86,560 AU)

Orbit about Galactic Center

Invariable-to-galactic plane inclination ~48.3°, to the ecliptic

Distance to

Galactic Center ~27,570 ly

Orbital speed ~211 km/s (~759,600 km/h)

Orbital period ~238 million years