Exoplanet · gas giant
HD 145457 b
HD 145457 b is a gas giant orbiting the star Kamuy. Its year lasts 176 Earth days. It was discovered in 2010 by the Radial Velocity method.
| Host star | Kamuy |
|---|---|
| Distance | 441.3 light-years (135.3 pc) |
| Orbital period | 176 days |
| Orbital radius | 0.762 AU |
| Eccentricity | 0.111 |
| Radius | 13.2 R⊕ · 1.18 R♃ |
| Mass (minimum) | 888 M⊕ · 2.79 M♃ |
| Density | 2.12 g/cm³ |
| Equilibrium temperature | 827 K (554 °C) |
| Stellar flux received | 77.8 × Earth |
| Discovery method | Radial Velocity |
| Discovery year | 2010 |
| Discovered by | Subaru Telescope |
Habitable zone
Inside the inner edge of the habitable zone: it receives 77.8 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 6.9° across: 13 times the Sun as we see it from Earth.
In the sky
Too faint for the naked eye (magnitude 6.57); binoculars will find it. Visible from the whole Northern Hemisphere and south to latitude 63° S. North of latitude 63° N it never sets. It stands highest at midnight in May, the best time to observe it.
Light's journey
The light you see tonight set out around the year 1585. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 7.8 million years.
Data: NASA Exoplanet Archive, PSCompPars. Its look in the simulation is a rendering based on the measured radius, mass and temperature.