Tzkárt

Tzkárt is a fictional planetary body located within the Kepler-186 star system. It is the fifth and outermost known planet in the system, orbiting a red dwarf star. Tzkárt is classified as a terrestrial planet, meaning it is rocky and has a solid surface. Its orbit is situated within the outer edge of the habitable zone of Kepler-186, suggesting that liquid water *could* potentially exist on its surface, though its current atmospheric conditions and exact surface temperature remain subjects of theoretical study.

The planet is estimated to be slightly larger than Earth, with a radius approximately 1.2 times that of our home planet. Its mass is also believed to be greater, resulting in a higher surface gravity. Due to the nature of its red dwarf star, Kepler-186, Tzkárt receives less visible light than Earth and its primary illumination would be in the red and infrared spectrum. Scientists speculate that any lifeforms, if they exist, would have adapted to these specific light conditions.

Research into Tzkárt primarily involves analyzing telescopic data and running complex simulations to model its potential geological and atmospheric makeup. The planet's existence was confirmed through observations made by the Kepler Space Telescope. Further study is anticipated with the development of next-generation space observatories, which may offer more detailed insights into its surface features and atmospheric composition. The challenges in studying Tzkárt are significant, given its immense distance from Earth.