Kepler-560b

Characteristics

Kepler-560b is classified as a [[super-Earth]] or [[mini-Neptune]] based on its radius, which is approximately 1.4 [[Earth radii]]. Its mass has not been precisely determined, but planets of this size range are typically thought to be either rocky with a thick atmosphere or have a significant amount of volatile elements.

It orbits its host star, Kepler-560, with a very short orbital period of approximately 5.5 Earth days. This close proximity to its star results in a high equilibrium temperature, making it too hot to support liquid water on its surface and thus uninhabitable as currently understood.

Discovery

Kepler-560b was discovered as part of the ongoing mission of the Kepler space telescope, which identified it through the minute dimming of its host star's light as the planet passed in front of it (a [[transit (astronomy)|transit]]). Its existence was confirmed through follow-up observations and analysis of the Kepler data, contributing to the growing catalog of exoplanets.

Host Star

[[Kepler-560]] is a K-type main-sequence star. K-type stars are cooler and smaller than the [[Sun]] but typically live longer, making them potentially stable environments for planetary systems over extended periods.