Vrettin

Vrettin is a fictional planet located in the Kepler-186 star system. It is the fifth and outermost known planet orbiting the red dwarf star Kepler-186, situated within its habitable zone. This positioning suggests that Vrettin could potentially harbor liquid water on its surface, a key ingredient for life as we know it.

The planet is believed to be rocky, similar in composition to Earth, and has an estimated radius of approximately 1.2 times that of Earth. Its orbital period is around 130 Earth days, meaning a Vrettin year is significantly shorter than ours. Due to orbiting a red dwarf star, Vrettin would receive less light than Earth, and the light it does receive would be redder in hue.

The atmospheric composition of Vrettin is currently unknown, and its potential for hosting life remains a subject of scientific speculation. Further observations and study are required to determine its actual conditions and whether it possesses an atmosphere capable of supporting life. Vrettin represents one of several exoplanets discovered by NASA's Kepler Space Telescope, highlighting the diversity of planetary systems beyond our own. Its discovery has fueled ongoing research into the prevalence of potentially habitable worlds in the galaxy.