Exoplanet · super-Earth
HD 164922 d
HD 164922 d is a super-Earth orbiting the star HD 164922. Its year lasts 12.5 Earth days. It was discovered in 2020 by the Radial Velocity method.
| Host star | HD 164922 |
|---|---|
| Distance | 71.8 light-years (22.0 pc) |
| Orbital period | 12.5 days |
| Orbital radius | 0.103 AU |
| Eccentricity | 0.120 |
| Radius | 1.83 R⊕ · 0.163 R♃ |
| Mass (minimum) | 4 M⊕ · 0.0126 M♃ |
| Density | 3.59 g/cm³ |
| Equilibrium temperature | 788 K (515 °C) |
| Stellar flux received | 66.9 × Earth |
| Discovery method | Radial Velocity |
| Discovery year | 2020 |
| Discovered by | Roque de los Muchachos Observatory |
Habitable zone
Inside the inner edge of the habitable zone: it receives 66.9 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 4.9° across: 9.2 times the Sun as we see it from Earth.
In the sky
Too faint for the naked eye (magnitude 7.01); binoculars will find it. Visible from the whole Northern Hemisphere and south to latitude 64° S. North of latitude 64° N it never sets. It stands highest at midnight in June, the best time to observe it.
Light's journey
The light you see tonight set out around the year 1954. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 1.3 million years.
Planets in the same system
- HD 164922 e 41.8-day orbit · 3.23 R⊕
- HD 164922 c 75.7-day orbit · 3.66 R⊕
- HD 164922 b 1,210-day orbit · 13.3 R⊕
Data: NASA Exoplanet Archive, PSCompPars. Its look in the simulation is a rendering based on the measured radius, mass and temperature.