Discovery | |
---|---|
Discovered by | Aldo S. Bonomo et al. |
Discovery date | 25 October 2011 |
Transit method | |
Orbital characteristics | |
0.0268 ± 0.0005 AU (4,009,000 ± 75,000 km)[1] | |
1.4857108 ± 0.0000002[1] d | |
Inclination | 87.22 ± 0.15[1] |
Star | Kepler-17 |
Physical characteristics | |
1.33 ± 0.04[1] RJ | |
Mass | 2.47 ± 0.10[1] MJ |
Mean density | 1.30 ± 0.14 g/cm3 (0.0470 ± 0.0051 lb/cu in)[1] |
3.54 ± 0.03 m/s2 (11.614 ± 0.098 ft/s2)[1] | |
Temperature | 2229+50 −58 K.[2] |
Kepler-17b is a planet in the orbit of star Kepler-17, first observed by the Kepler spacecraft observatory in 2011. Kepler-17b is a gas giant nearly 2.45 times the mass of Jupiter, and is sometimes described as a "super-Jupiter".
The planet is likely to be tidally locked to the parent star. In 2015, the planetary nightside temperature was estimated to be equal to 2229+50
−58 K.[2]
The study in 2012, utilizing a Rossiter–McLaughlin effect, have determined the planetary orbit is probably aligned with the equatorial plane of the star, misalignment equal to 0±15°.[3]