HAT-P-11b
| Size comparison of Neptune with HAT-P-11b (gray). | |
| Discovery | |
|---|---|
| Discovered by | Bakos et al. | 
| Discovery site | Cambridge, Massachusetts | 
| Discovery date | 2 January 2009 | 
| Transit (HATNet) | |
| Orbital characteristics | |
| Apastron | 0.0637+0.0020 −0.0019 AU | 
| Periastron | 0.0413+0.0018 −0.0019 AU | 
| 0.05254+0.00064 −0.00066 AU | |
| Eccentricity | 0.218+0.034 −0.031 | 
| 4.887802443+0.000000034 −0.000000030 d | |
| Inclination | 89.05+0.15 −0.09 | 
| 2454957.15+0.17 −0.20 | |
| 19+14 −16 | |
| Semi-amplitude | 10.42+0.64 −0.66 | 
| Star | HAT-P-11 | 
| Physical characteristics | |
| 4.36±0.06 R🜨 | |
| Mass | 23.4±1.5 ME | 
| Mean density | 1.44 g/cm3 | 
| 1.20 g | |
HAT-P-11b (or Kepler-3b) is an extrasolar planet orbiting the star HAT-P-11. It was discovered by the HATNet Project team in 2009 using the transit method, and submitted for publication on 2 January 2009.
This planet is located approximately 123 light-years (38 pc) distant from Earth.