Exoplanet · gas giant
HD 21411 b
HD 21411 b is a gas giant orbiting the star HD 21411. Its year lasts 84.3 Earth days. It was discovered in 2019 by the Radial Velocity method.
| Host star | HD 21411 |
|---|---|
| Distance | 95.0 light-years (29.1 pc) |
| Orbital period | 84.3 days |
| Orbital radius | 0.362 AU |
| Eccentricity | 0.400 |
| Radius | 9.52 R⊕ · 0.849 R♃ |
| Mass (minimum) | 65.9 M⊕ · 0.207 M♃ |
| Density | 0.42 g/cm³ |
| Equilibrium temperature | 408 K (135 °C) |
| Stellar flux received | 4.14 × Earth |
| Discovery method | Radial Velocity |
| Discovery year | 2019 |
| Discovered by | Las Campanas Observatory |
Habitable zone
Inside the inner edge of the habitable zone: it receives 4.14 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: 2.3 times the Sun as we see it from Earth.
In the sky
Too faint for the naked eye (magnitude 7.88); binoculars will find it. Visible from the whole Southern Hemisphere and north to latitude 59° N. South of latitude 59° S it never sets. It stands highest at midnight in November, the best time to observe it.
Light's journey
The light you see tonight set out around the year 1931. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 1.7 million years.
Data: NASA Exoplanet Archive, PSCompPars. Its look in the simulation is a rendering based on the measured radius, mass and temperature.