Kepler-11e
| Size comparison of Kepler-11e (gray) with Neptune. | |
| Discovery | |
|---|---|
| Discovery date | 2 February 2011 | 
| Transit (Kepler Mission) | |
| Orbital characteristics | |
| 0.194 AU (29,000,000 km) | |
| 31.99590 d | |
| Inclination | 88.8 | 
| Star | Kepler-11 (KOI-157) | 
| Physical characteristics | |
| 4.52 (± 0.43) R🜨 | |
| Mass | 8.4 +2.5 −1.9 M🜨 | 
| Mean density | 0.5 (± 0.2) g cm−3 | 
| Temperature | 617 K (344 °C; 651 °F) | 
Kepler-11e is an exoplanet (extrasolar planet) discovered in the orbit of the sunlike star Kepler-11. It is the fourth of six planets around Kepler-11 discovered by NASA's Kepler space telescope. Kepler-11e was found by using the transit method, in which the dimming effect that a planet causes as it crosses in front of its star is measured. Kepler-11e is most likely a gas giant like Neptune, having a density that is less than that of Saturn, the least dense planet in the Solar System. Its low density can probably be attributed to a large hydrogen and helium atmosphere. Kepler-11e has a mass eight times of Earth's mass and a radius 4.5 times that of Earth. The planet orbits its star every 31 days in an ellipse that would fit within the orbit of Mercury. Kepler-11e was announced on February 2, 2011 with its five sister planets after it was confirmed by several observatories.