Virkania

Virkania is a planet located within the Vargalos star system, approximately 35 light‑years from Earth. It was first recorded by the Interstellar Survey Initiative in 2147 during a routine stellar mapping mission. The planet orbits its G‑type primary star at a distance that places it in the system’s habitable zone, with a surface temperature range conducive to liquid water on substantially large areas.

Geologically, Virkania features a layered mantle predominated by silicate minerals, with extensive basaltic volcanic plains covering roughly 48% of its surface. The planet’s crust is marked by frequent tectonic activity, producing a series of ringed mountain ranges and deep oceanic trenches. Notable among its geological formations are the luminous “Aurora Canyons,” deep fissures that emit bioluminescent glows caused by microbial metabolic processes within the rock.

The biosphere of Virkania hosts diverse flora and fauna adapted to its humid, moderate climate. The dominant vegetation is the canopy-dwelling “Glosswing fern,” a photosynthetic plant that releases a fragrant pollen used in interstellar trade. Fauna include ornithoid creatures known as “Silverbirds,” which possess reflective plumage and a complex mating ritual involving synchronized wing-flickering. Scientific surveys have recorded several unique species of amphibious mammals that thrive in the planet’s extensive wetlands.

Human research missions have concentrated on Virkania’s potential for agricultural bioengineering and sustainable energy harvesting. Its abundant geothermal vents and geothermal gradients have attracted interest for clean energy extraction, while the planet’s native biochemistries are studied for biofuel development. International collaboration agreements were signed in 2163, designating Virkania as a protected research outpost and encouraging cooperative study of its natural resources and ecological systems.