Exoplanet · Neptune-like planet
HD 10180 f
HD 10180 f is a Neptune-like planet orbiting the star HD 10180. Its year lasts 123 Earth days. It was discovered in 2010 by the Radial Velocity method.
| Host star | HD 10180 |
|---|---|
| Distance | 127.1 light-years (39.0 pc) |
| Orbital period | 123 days |
| Orbital radius | 0.493 AU |
| Eccentricity | 0.119 |
| Radius | 5.24 R⊕ · 0.467 R♃ |
| Mass | 23.9 M⊕ · 0.0752 M♃ |
| Density | 0.913 g/cm³ |
| Equilibrium temperature | 428 K (154 °C) |
| Stellar flux received | 6.13 × Earth |
| Discovery method | Radial Velocity |
| Discovery year | 2010 |
| Discovered by | La Silla Observatory |
Habitable zone
Inside the inner edge of the habitable zone: it receives 6.13 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 1.2° across: 2.2 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 29° N. South of latitude 29° S it never sets. It stands highest at midnight in October, the best time to observe it.
Light's journey
The light you see tonight set out around the year 1899. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 2.3 million years.
Planets in the same system
- HD 10180 c 5.76-day orbit
- HD 10180 d 16.4-day orbit
- HD 10180 e 49.7-day orbit · 5.39 R⊕
- HD 10180 g 605-day orbit
- HD 10180 h 2,210-day orbit · 9.4 R⊕
Data: NASA Exoplanet Archive, PSCompPars. Its look in the simulation is a rendering based on the measured radius, mass and temperature.