Miri system
It is in orbit of a class III, type G7 (Yellow) star called Miri. The other objects in this star system are
- 1)a hot rock ball of a planet, it's orbit is approximately 33 million km, diameter of 1273.5 km (791.5 miles).
- 2)a rock ball of a planet, it's orbit is approximately 62 million km, diameter of 8,525 km (5,328 miles).
- 3)a hostile greenhouse planet, it's orbit is approximately 112 million km, diameter of 11,109 km (6,943 miles).
- 4)a class M planet (Miri IV), it's orbit is approximately 149 million km, diameter of 12,664 km (7,915 miles). See Starfleet Intelligence File 2266-28473, Miri.
- 5)a large gas giant, it's orbit is approximately 202 million km.
- 6)a medium gas giant, it's orbit is approximately 257 million km
- 7)an icy rock ball of a planet, it's orbit is approximately 326 million km, diameter of 5,994 km (3,746 miles).
|
| Serellan Sector |
|---|
| Trinity Sector |
| Jenatris Cloud Sector |
| (Sector 118 map) |
| Territory |
| Local Species |
| Stellar Phenomenae |
| Federation Presence |
|
|
| Miri system | Star · I · II · III · IV · V · VI · VII |
The Miri system is a system of 7 planets orbiting a G type star in the Trinity Sector. It is approximately 4 lightyears from Starbase 118 in the direction of Epsilon Outpost #11. It is in close proximity to the Gamma Taboa system, which is less than a light year away towards the Outpost.
Of the seven planets, the fourth is inhabited and has applied to join the Federation. The first and second planets lack atmosphere whilst the third has a runaway greenhouse effect. The fifth and sixth planets are gas giants whilst the seventh is an ice dwarf.
Partly due to the negative conditions encountered during the first contact with the Human colony on Miri IV and certain problems plaguing the records department for deep space records, all the original information for this system was incorrectly filed under Ophiucus 70 system. Ophiucus 70 is roughly equidistant in the opposite direction from Sol.