Exoplanet · mini-Neptune
HD 56414 b
HD 56414 b is a mini-Neptune orbiting the star HD 56414. Its year lasts 29 Earth days. It was discovered in 2022 by the Transit method.
| Host star | HD 56414 |
|---|---|
| Distance | 887.9 light-years (272.2 pc) |
| Orbital period | 29 days |
| Orbital radius | 0.229 AU |
| Eccentricity | 0.680 |
| Radius | 3.71 R⊕ · 0.331 R♃ |
| Mass | 13.3 M⊕ · 0.0418 M♃ (estimated from the radius) |
| Density | 1.43 g/cm³ |
| Equilibrium temperature | 1,133 K (860 °C) |
| Stellar flux received | 1,610 × Earth |
| Discovery method | Transit |
| Discovery year | 2022 |
| Discovered by | Transiting Exoplanet Survey Satellite (TESS) |
Habitable zone
Inside the inner edge of the habitable zone: it receives 1,610 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 4.1° across: 7.6 times the Sun as we see it from Earth.
In the sky
A telescope is needed to see it: its apparent magnitude is 9.24. Visible from the whole Southern Hemisphere and north to latitude 21° N. South of latitude 21° S it never sets. It stands highest at midnight in January, the best time to observe it.
Light's journey
The light you see tonight set out around the year 1138. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 16 million years.
Data: NASA Exoplanet Archive, PSCompPars. Its look in the simulation is a rendering based on the measured radius, mass and temperature.