TOI-1117 is 547 light-years from the Sun. The NASA Exoplanet Archive lists 3 planets around this G5 V star; the first was found in 2025 by transit (Transiting Exoplanet Survey Satellite (TESS)).
Fly there in 3DTOI-1117 b goes round its star every 2.23 days, 39 times as often as Mercury goes round the Sun.
| Spectral type | G5 V |
| Surface temperature | 5,635 K |
| Mass | 0.97 solar masses |
| Radius | 1.05 solar radii |
| Luminosity | 0.36 times the Sun |
| Apparent magnitude | 11.016 |
| Age | about 4.42 billion years |
| Distance from the Sun | 546.6 light-years (167.6 parsecs) |
| Position (J2000) | RA 273.6021°, Dec -66.4200° |
| Constellation | Pavo |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| TOI-1117 b | 2.23 days | 0.0330 AU | 2.46 R⊕ | 8.9 M⊕ | Transit, 2025 |
| TOI-1117 c | 4.58 days | 0.0534 AU | 2.91 R⊕ estimated | 8.78 M⊕ minimum | Radial Velocity, 2025 |
| TOI-1117 d | 8.66 days | 0.0817 AU | 3.27 R⊕ estimated | 10.71 M⊕ minimum | Radial Velocity, 2025 |
Values are the NASA Exoplanet Archive’s composite parameters. A radius marked estimated comes from a mass–radius relation; a mass marked minimum is M sin i. Planet sizes and colours in the 3D view are renderings: none of these worlds has been photographed as more than a point of light.
For a star of 5,635 K, 0.36 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 0.58 to 1.02 AU. None of its known planets orbits inside it. The zone says how much starlight arrives, not whether a planet has water or air. The edges follow Kopparapu et al. (2014), as the 3D view draws them.
The light you see left 547 years ago, around 1480.