Neorakidura

Neorakidura is a fictional planet located in the Kepler-186 system, a star system approximately 500 light-years from Earth. Discovered by exoplanetology researchers, Neorakidura is a terrestrial planet, meaning it is primarily composed of silicate rocks and metals. Its size is comparable to Earth, with a radius estimated to be around 1.2 times that of our home planet.

The planet orbits within the habitable zone of its star, Kepler-186f, a red dwarf. This orbital position suggests that liquid water could potentially exist on Neorakidura's surface, a key ingredient for life as we understand it. However, the atmospheric composition of Neorakidura remains largely unknown, which would significantly influence its surface temperature and habitability. Red dwarf stars are also known for their stellar flares, which could pose a challenge to life developing or surviving on nearby planets.

Current research on Neorakidura is based on data gathered by space telescopes analyzing the light passing through its atmosphere during transits. Further observations are needed to determine its atmospheric pressure, temperature, and the presence of biosignatures. The planet's existence highlights the ongoing efforts in the search for exoplanets that might harbor life beyond our solar system. The study of Neorakidura contributes to our understanding of planetary formation and the conditions necessary for habitability in diverse stellar environments.