Discovery | |
---|---|
Discovered by | Kepler spacecraft[1] |
Discovery date | 2017 Shallue et al.[2][1] |
Transit[2] and deep learning, a class of machine learning algorithms.[1] | |
Orbital characteristics | |
0.107+0.025 −0.040[1] AU | |
14.44912±0.00020[2] d | |
Inclination | 89.20 +0.59 −1.30[2] |
Star | Kepler-90 |
Physical characteristics | |
1.32±0.21[2] R🜨 | |
Temperature | 709 K (436 °C; 817 °F)[2] |
Kepler-90i (also known by its Kepler Object of Interest designation KOI-351.08)[2] is a super-Earth exoplanet with a radius 1.32[2] times that of Earth, orbiting the early G-type main sequence star Kepler-90 every 14.45 days, discovered by NASA's Kepler spacecraft.[1][3] It is located about 2,840 light-years (870 parsecs, or nearly 2.4078×1016 km) from Earth in the constellation Draco. The exoplanet is the eighth in the star's multiplanetary system. As of December 2017, Kepler-90 is the star hosting the most exoplanets found. Kepler-90i was found with the transit method, in which the dimming effect that a planet causes as it crosses in front of its star is measured, and by a newly utilized computer tool, deep learning, a class of machine learning algorithms.[1][4][5]