Exoplanet · Neptune-like planet
TOI-333 b
TOI-333 b is a Neptune-like planet orbiting the star TOI-333. Its year lasts 3.79 Earth days. It was discovered in 2025 by the Transit method.
| Host star | TOI-333 |
|---|---|
| Distance | 1,149 light-years (352.3 pc) |
| Orbital period | 3.79 days |
| Orbital radius | 0.049 AU |
| Eccentricity | 0.000 |
| Radius | 4.26 R⊕ · 0.38 R♃ |
| Mass | 20.1 M⊕ · 0.0632 M♃ |
| Density | 1.42 g/cm³ |
| Surface gravity | 1.11 × Earth |
| Equilibrium temperature | 1,445 K (1,172 °C) |
| Stellar flux received | 650 × Earth |
| Discovery method | Transit |
| Discovery year | 2025 |
| Discovered by | Transiting Exoplanet Survey Satellite (TESS) |
Habitable zone
Inside the inner edge of the habitable zone: it receives 650 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 12° across: 22 times the Sun as we see it from Earth.
In the sky
A telescope is needed to see it: its apparent magnitude is 12.27. Visible from the whole Southern Hemisphere and north to latitude 49° N. South of latitude 49° S it never sets. It stands highest at midnight in September, the best time to observe it.
Light's journey
The light you see tonight set out around the year 877. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 20 million years.
Data: NASA Exoplanet Archive, PSCompPars. Its look in the simulation is a rendering based on the measured radius, mass and temperature.