Berijis (Planet)
Berijis
General Information
| Details | Data |
|---|---|
| Average Distance From Star | 21.5 AU (2,877 million km) |
| Eccentricity | 0.04 |
| Orbital Period (sidereal) | 34434.22 d |
| Satellites | 45 |
| Mean Radius | 25,362 km (3.42 Utopias) |
| Surface Area | 8,083,079,689 km2 |
| Mass | 8.68E+25 kg (11.704 Utopias) |
| Mean Density | 1.27 g/cm3 (0.29 Utopias) |
| Surface Gravity | 1 Utopian G |
| Escape Velocity | 21.37 km/s |
| Sidereal Rotation Period | 0.72 d |
| Axial tilt | 297.77° |
| Albedo | 0.30 |
| Temperature | 51 K |
| Surface temp | 92 K |
| ---- | ---- |
Berijis
Berijis is the sixth and second largest planet in the Helios System. It’s surface is covered by a pale teal shroud of clouds saturated with volatile “ices”. Berijis is one of two planets in the Helios system with a retrograde rotation, but is unique in that its high axial tilt of 97.77° causes the planet’s poles to be parallel to Berijis’ orbital plane. This causes erratic storm formation and high wind speed on Berijis compared to its sister planet, Kayvon.
Berijis was discovered by Meridian astronomers in 1754, who named it after the ancient Meridian deity Berjis. Over the next two centuries, the thin ring of Berijis and its 45 natural satellites were discovered. Of its many satellites, the five largest are considered major moons:
Kari, Oru, Hilal, Guantian, and Sezu. Berijis is the least visited planet in the Helios system, with only a few dozen satellite visits since 1964 when it was first Surveyed by the Meridian Commonwealth. In 2025 however, the state of Kjanu launched the Canary-1 Satellite as part of a mission to survey the moons of Berijis.
Provide by ArsonistGlaceon(User)