Vorén

Vorén is a fictional planet located in the Kepler-186 system, approximately 500 light-years from Earth. It is the fifth planet in the system and resides within the habitable zone of its star, Kepler-186f, a red dwarf. Initial telescopic observations suggest Vorén is a terrestrial planet, potentially rocky, with a diameter roughly 1.2 times that of Earth. Its mass is estimated to be around 1.5 Earth masses, indicating a similar density.

The planet's atmosphere is a subject of ongoing scientific inquiry. Spectroscopic analysis has detected trace amounts of oxygen and methane, which could be biosignatures. However, these findings are not conclusive, and further investigation is required to determine their origin. The presence of liquid water on the surface is considered plausible due to its location within the habitable zone. Temperature estimates suggest an average surface temperature that could support liquid water, though variations due to atmospheric composition and planetary albedo are possible.

Vorén's orbital period is approximately 130 Earth days. It is tidally locked to its star, meaning one side perpetually faces Kepler-186f while the other remains in darkness. This phenomenon would create extreme temperature differences between the two hemispheres, with a potential temperate band along the terminator. Research into Vorén is primarily conducted through advanced telescopic observations and theoretical modeling. No crewed missions have been sent to Vorén, and its existence remains within the realm of exoplanetary discovery.