Exoplanet · super-Earth
HD 108236 b
HD 108236 b is a super-Earth orbiting the star HD 108236. Its year lasts 3.8 Earth days. It was discovered in 2020 by the Transit method.
| Host star | HD 108236 |
|---|---|
| Distance | 210.7 light-years (64.6 pc) |
| Orbital period | 3.8 days |
| Orbital radius | 0.0453 AU |
| Eccentricity | 0.045 |
| Radius | 1.62 R⊕ · 0.144 R♃ |
| Mass | 3.24 M⊕ · 0.0102 M♃ (estimated from the radius) |
| Density | 4.23 g/cm³ |
| Equilibrium temperature | 1,099 K (826 °C) |
| Stellar flux received | 312 × Earth |
| Discovery method | Transit |
| Discovery year | 2020 |
| Discovered by | Transiting Exoplanet Survey Satellite (TESS) |
Habitable zone
Inside the inner edge of the habitable zone: it receives 312 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 10° across: 19 times the Sun as we see it from Earth.
In the sky
A telescope is needed to see it: its apparent magnitude is 9.25. Visible from the whole Southern Hemisphere and north to latitude 39° N. South of latitude 39° S it never sets. It stands highest at midnight in March, the best time to observe it.
Light's journey
The light you see tonight set out around the year 1815. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 3.7 million years.
Planets in the same system
- HD 108236 c 6.2-day orbit · 2.07 R⊕
- TOI-1233.01 14.2-day orbit · 2.54 R⊕
- HD 108236 e 19.6-day orbit · 3.08 R⊕
- HD 108236 f 29.5-day orbit · 2.02 R⊕
Data: NASA Exoplanet Archive, PSCompPars. Its look in the simulation is a rendering based on the measured radius, mass and temperature.