Exoplanet · gas giant
HIP 14810 b
HIP 14810 b is a gas giant orbiting the star HIP 14810. Its year lasts 6.67 Earth days. It was discovered in 2005 by the Radial Velocity method.
| Host star | HIP 14810 |
|---|---|
| Distance | 164.6 light-years (50.5 pc) |
| Orbital period | 6.67 days |
| Orbital radius | 0.0696 AU |
| Eccentricity | 0.144 |
| Radius | 13 R⊕ · 1.16 R♃ |
| Mass (minimum) | 1,240 M⊕ · 3.9 M♃ |
| Density | 3.1 g/cm³ |
| Equilibrium temperature | 1,048 K (775 °C) |
| Stellar flux received | 202 × Earth |
| Discovery method | Radial Velocity |
| Discovery year | 2005 |
| Discovered by | W. M. Keck Observatory |
Habitable zone
Inside the inner edge of the habitable zone: it receives 202 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 8.2° across: 15 times the Sun as we see it from Earth.
In the sky
Too faint for the naked eye (magnitude 8.52); binoculars will find it. Visible from the whole Northern Hemisphere and south to latitude 69° S. North of latitude 69° N it never sets. It stands highest at midnight in November, the best time to observe it.
Light's journey
The light you see tonight set out around the year 1861. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 2.9 million years.
Planets in the same system
- HIP 14810 c 148-day orbit · 13.6 R⊕
- HIP 14810 d 982-day orbit · 14.1 R⊕
Data: NASA Exoplanet Archive, PSCompPars. Its look in the simulation is a rendering based on the measured radius, mass and temperature.