Exoplanet · gas giant
HD 142415 b
HD 142415 b is a gas giant orbiting the star HD 142415. Its year lasts 386 Earth days. It was discovered in 2003 by the Radial Velocity method.
| Host star | HD 142415 |
|---|---|
| Distance | 115.9 light-years (35.5 pc) |
| Orbital period | 386 days |
| Orbital radius | 1.06 AU |
| Eccentricity | 0.500 |
| Radius | 13.5 R⊕ · 1.2 R♃ |
| Mass (minimum) | 531 M⊕ · 1.67 M♃ |
| Density | 1.19 g/cm³ |
| Equilibrium temperature | 284 K (11 °C) |
| Stellar flux received | 1.02 × Earth |
| Discovery method | Radial Velocity |
| Discovery year | 2003 |
| Discovered by | La Silla Observatory |
Habitable zone
Inside its star's habitable zone: it receives enough light for liquid water to exist on its surface under a suitable atmosphere.
Its star in the sky
In the planet's sky its star is a disc 0.52° across: 0.98 times the Sun as we see it from Earth.
In the sky
Too faint for the naked eye (magnitude 7.33); binoculars will find it. Visible from the whole Southern Hemisphere and north to latitude 30° N. South of latitude 30° S 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 1910. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 2.1 million years.
Data: NASA Exoplanet Archive, PSCompPars. Its look in the simulation is a rendering based on the measured radius, mass and temperature.