Exoplanet · gas giant
KELT-11 b
KELT-11 b is a gas giant orbiting the star KELT-11. Its year lasts 4.74 Earth days. It was discovered in 2017 by the Transit method.
| Host star | KELT-11 |
|---|---|
| Distance | 323.4 light-years (99.2 pc) |
| Orbital period | 4.74 days |
| Orbital radius | 0.0623 AU |
| Eccentricity | 0.000 |
| Radius | 15.1 R⊕ · 1.35 R♃ |
| Mass | 65.2 M⊕ · 0.205 M♃ |
| Density | 0.093 g/cm³ |
| Surface gravity | 0.285 × Earth |
| Equilibrium temperature | 1,712 K (1,439 °C) |
| Stellar flux received | 1,430 × Earth |
| Discovery method | Transit |
| Discovery year | 2017 |
| Discovered by | KELT-South |
Habitable zone
Inside the inner edge of the habitable zone: it receives 1,430 times the light the Earth does, too hot to keep liquid water on its surface.
Its star in the sky
In the planet's sky its star is a disc 23° across: 43 times the Sun as we see it from Earth.
In the sky
Too faint for the naked eye (magnitude 8.04); binoculars will find it. Visible from the whole Southern Hemisphere and north to latitude 81° N. It stands highest at midnight in March, the best time to observe it.
Light's journey
The light you see tonight set out around the year 1703. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 5.7 million years.
Data: NASA Exoplanet Archive, PSCompPars. Its look in the simulation is a rendering based on the measured radius, mass and temperature.