Kepler-1520

Kepler-1520 (initially published as KIC 12557548) is a K-type main-sequence star located in the constellation Cygnus. The star is particularly important, as measurements taken by the Kepler spacecraft indicate that the variations in the star's light curve cover a range from about 0.2% to 1.3% of the star's light being blocked.^[2] This indicates that there may be a rapidly disintegrating planet, a prediction not yet conclusively confirmed, in orbit around the star, losing mass at a rate of 1 Earth mass every billion years.^[2] The planet itself is about 0.1 Earth masses,^[8] or just twice the mass of Mercury, and is expected to disintegrate in about 100^[8]-200 million years.^[2] The planet orbits its star in just 15.7 hours,^[2] at a distance only two stellar diameters away from the star's surface,^[9] and has an estimated effective temperature of about 2255 K.^[8] The orbital period of the planet is one of the shortest ever detected in the history of the extrasolar planet search.^[10] In 2016, the planet was confirmed as part of a data release by the Kepler spacecraft.

Nomenclature and history[]

Prior to Kepler observation, Kepler-1520 had the 2MASS catalogue number 2MASS J19235189+5130170. In the Kepler Input Catalog it has the designation of KIC 12557548, and when it was found to have transiting planet candidates it was given the Kepler object of interest number of KOI-3794.

The star's planetary companion were discovered by NASA's Kepler Mission, a mission tasked with discovering planets in transit around their stars. The transit method that Kepler uses involves detecting dips in brightness in stars. These dips in brightness can be interpreted as planets whose orbits move in front of their stars from the perspective of Earth. The name Kepler-1520 derives directly from the fact that the star is the catalogued 1,520th star discovered by Kepler to have confirmed planets.

The designation b, derive from the order of discovery. The designation of b is given to the first planet orbiting a given star, followed by the other lowercase letters of the alphabet.^[11] In the case of Kepler-1520, there was only one planet detected, so only the letter b is used.

Stellar characteristics[]

Kepler-1520 is a K-type star that is approximately 76% the mass of and 71% the radius of the Sun. It has a surface temperature of 4677 K and is about 4.47 billion years old.^[5] In comparison, the Sun is about 4.6 billion years old^[12] and has a surface temperature of 5778 K.^[13]

The star's apparent magnitude, or how bright it appears from Earth's perspective, is 15. Therefore, it is too dim to be seen with the naked eye.

Planetary system[]