Exoplanet · gas giant
HIP 63242 b
HIP 63242 b is a gas giant orbiting the star HIP 63242. Its year lasts 125 Earth days. It was discovered in 2013 by the Radial Velocity method.
| Host star | HIP 63242 |
|---|---|
| Distance | 510.3 light-years (156.5 pc) |
| Orbital period | 125 days |
| Orbital radius | 0.565 AU |
| Eccentricity | 0.230 |
| Radius | 12.5 R⊕ · 1.12 R♃ |
| Mass (minimum) | 2,920 M⊕ · 9.18 M♃ |
| Density | 8.21 g/cm³ |
| Equilibrium temperature | 993 K (720 °C) |
| Stellar flux received | 134 × Earth |
| Discovery method | Radial Velocity |
| Discovery year | 2013 |
| Discovered by | Multiple Observatories |
Habitable zone
Inside the inner edge of the habitable zone: it receives 134 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 9.7° across: 18 times the Sun as we see it from Earth.
In the sky
Too faint for the naked eye (magnitude 6.86); binoculars will find it. Visible from the whole Southern Hemisphere and north to latitude 24° N. South of latitude 24° S it never sets. It stands highest at midnight in April, the best time to observe it.
Light's journey
The light you see tonight set out around the year 1516. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 9.1 million years.
Data: NASA Exoplanet Archive, PSCompPars. Its look in the simulation is a rendering based on the measured radius, mass and temperature.