Exoplanet · gas giant
Kepler-88 d
Kepler-88 d is a gas giant orbiting the star KOI-142. Its year lasts 1,400 Earth days. It was discovered in 2020 by the Radial Velocity method.
| Host star | KOI-142 |
|---|---|
| Distance | 1,229 light-years (376.9 pc) |
| Orbital period | 3.84 years |
| Orbital radius | 2.47 AU |
| Eccentricity | 0.410 |
| Radius | 13.1 R⊕ · 1.17 R♃ |
| Mass | 965 M⊕ · 3.04 M♃ |
| Density | 2.36 g/cm³ |
| Equilibrium temperature | 159 K (-114 °C) |
| Stellar flux received | 0.112 × Earth |
| Discovery method | Radial Velocity |
| Discovery year | 2020 |
| Discovered by | W. M. Keck Observatory |
Habitable zone
Beyond the habitable zone: it receives only %11 of the light the Earth does, a frozen world.
Its star in the sky
In the planet's sky its star is a disc 0.19° across: 0.36 times the Sun as we see it from Earth.
In the sky
A telescope is needed to see it: its apparent magnitude is 13.21. Visible from the whole Northern Hemisphere and south to latitude 49° S. North of latitude 49° N it never sets. It stands highest at midnight in July, the best time to observe it.
Light's journey
The light you see tonight set out around the year 797. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 22 million years.
Planets in the same system
Data: NASA Exoplanet Archive, PSCompPars. Its look in the simulation is a rendering based on the measured radius, mass and temperature.