description Kepler-36c Overview
Kepler-36c is a transiting exoplanet orbiting the star Kepler-36 and was reported in 2012 from observations by NASA's Kepler mission. It is larger and less dense than neighboring Kepler-36b, indicating a substantial volatile envelope rather than a predominantly rocky composition. The two planets have markedly different densities despite exceptionally close orbital spacing, and their mutual gravitational effects produce measurable transit-timing variations.
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What type of planet is Kepler-36c?
Kepler-36c is a transiting exoplanet that is larger and less dense than its neighboring planet, indicating it has a substantial volatile envelope. This means it is likely a gas-rich mini-Neptune rather than a predominantly rocky world.
When was Kepler-36c discovered?
The planet was reported in 2012 based on observations made by NASA's Kepler mission. The discovery was notable because of the extreme proximity of the planets in the system.
What makes the Kepler-36 system unique?
The Kepler-36 system is remarkable because planets Kepler-36b and Kepler-36c have wildly different compositions despite orbiting extremely close to one another. They pass within a fraction of the distance between Earth and the Moon.
What star does Kepler-36c orbit?
Kepler-36c orbits a subgiant star named Kepler-36 that is located thousands of light-years away from Earth. The star is in the late stages of its stellar life.
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