Kepler-69c is an exoplanet located in the habitable zone of its star, exhibiting characteristics that make it a candidate for hosting liquid water and possibly life.
Overview
The Star Kepler 69
Exploration Missions
Comparison With Earth
Scientific Importance
Habitability Potential
Discovery Of Kepler 69 C
Future Research Directions
Characteristics Of Kepler 69 C
James Webb Space Telescope
Temperature
Atmosphere
Light-year
Discovery
Interest
Universe
Gravity
Liquid
๐ Kepler-69c is located about 2,700 light-years away from Earth in the constellation Cygnus.
๐ It is classified as a super-Earth due to its size being larger than Earth's but smaller than that of Neptune.
๐ง Kepler-69c orbits within the habitable zone of its host star, which could allow for liquid water to exist on its surface.
โญ The host star, Kepler-69, is a G-type star similar to our Sun, with a temperature of around 5,700 K.
๐ญ Kepler-69c was discovered by NASA's Kepler Space Telescope in 2013.
๐ช Its radius is approximately 1.7 times that of Earth, suggesting it may have a rocky composition.
๐ก๏ธ The estimated equilibrium temperature of Kepler-69c is around 120ยฐC (248ยฐF), potentially indicating a warm atmosphere.
๐ It takes approximately 13.7 days to complete one orbit around its star.
๐ The planet is part of a planetary system that includes at least one other confirmed planet, Kepler-69b.
๐ฑ Scientists are particularly interested in Kepler-69c as it offers possibilities for future studies regarding habitability.