Exoplanet · gas giant
HD 42012 b
HD 42012 b is a gas giant orbiting the star HD 42012. Its year lasts 858 Earth days. It was discovered in 2017 by the Radial Velocity method.
| Host star | HD 42012 |
|---|---|
| Distance | 120.0 light-years (36.8 pc) |
| Orbital period | 2.35 years |
| Orbital radius | 1.67 AU |
| Eccentricity | 0.200 |
| Radius | 13.5 R⊕ · 1.2 R♃ |
| Mass (minimum) | 509 M⊕ · 1.6 M♃ |
| Density | 1.14 g/cm³ |
| Equilibrium temperature | 183 K (-91 °C) |
| Stellar flux received | 0.193 × Earth |
| Discovery method | Radial Velocity |
| Discovery year | 2017 |
| Discovered by | Haute-Provence Observatory |
Habitable zone
Beyond the habitable zone: it receives only %19 of the light the Earth does, a frozen world.
Its star in the sky
In the planet's sky its star is a disc 0.26° across: 0.49 times the Sun as we see it from Earth.
In the sky
Too faint for the naked eye (magnitude 8.44); binoculars will find it. Visible from the whole Northern Hemisphere and south to latitude 56° S. North of latitude 56° N it never sets. It stands highest at midnight in December, the best time to observe it.
Light's journey
The light you see tonight set out around the year 1906. 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.