Exoplanet · gas giant
HD 96167 b
HD 96167 b is a gas giant orbiting the star HD 96167. Its year lasts 498 Earth days. It was discovered in 2009 by the Radial Velocity method.
| Host star | HD 96167 |
|---|---|
| Distance | 278.2 light-years (85.3 pc) |
| Orbital period | 498 days |
| Orbital radius | 1.33 AU |
| Eccentricity | 0.685 |
| Radius | 14 R⊕ · 1.25 R♃ |
| Mass (minimum) | 228 M⊕ · 0.717 M♃ |
| Density | 0.456 g/cm³ |
| Equilibrium temperature | 334 K (60 °C) |
| Stellar flux received | 2.09 × Earth |
| Discovery method | Radial Velocity |
| Discovery year | 2009 |
| Discovered by | W. M. Keck Observatory |
Habitable zone
Inside the inner edge of the habitable zone: it receives 2.09 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 0.78° across: 1.5 times the Sun as we see it from Earth.
In the sky
Too faint for the naked eye (magnitude 8.09); binoculars will find it. Visible from the whole Southern Hemisphere and north to latitude 80° N. South of latitude 80° S it never sets. 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 1748. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 4.9 million years.
Data: NASA Exoplanet Archive, PSCompPars. Its look in the simulation is a rendering based on the measured radius, mass and temperature.