Havrikas

Havrikas is a fictional planet located in the Kepler-186 star system, a red dwarf star approximately 580 light-years from Earth. Discovered by the Kepler space telescope, Havrikas gained prominence due to its position within the star's habitable zone, the region where liquid water could potentially exist on the planet's surface.

The planet is estimated to be roughly Earth-sized, with a radius only slightly larger than our own. Its orbital period around Kepler-186 is approximately 130 days. Due to the dimmer nature of its red dwarf star, Havrikas receives less stellar radiation compared to Earth, which may influence its atmospheric composition and temperature.

Current scientific understanding suggests that if Havrikas possesses an atmosphere, its surface temperature could support liquid water, a key ingredient for life as we know it. However, no direct observations of its atmosphere or surface features have been made. The potential for habitability remains a subject of ongoing research and speculation among astronomers and astrobiologists. Further observations, potentially with future advanced telescopes, are needed to confirm the presence of an atmosphere and to search for biosignatures. The existence of Havrikas highlights the growing number of exoplanets being discovered that reside within the habitable zones of their stars.