TOI-6695 is 922 light-years from the Sun. The NASA Exoplanet Archive lists 2 planets around this F5V-G0V star; the first was found in 2025 by transit (Transiting Exoplanet Survey Satellite (TESS)).
Fly there in 3DTOI-6695 b goes round its star every 80.4 days, 1.1 times as often as Mercury goes round the Sun.
| Spectral type | F5V-G0V |
| Surface temperature | 6,400 K |
| Mass | 1.338 solar masses |
| Radius | 1.517 solar radii |
| Luminosity | 3.47 times the Sun |
| Apparent magnitude | 10.768 |
| Age | about 2.1 billion years |
| Distance from the Sun | 921.5 light-years (282.5 parsecs) |
| Position (J2000) | RA 129.5720°, Dec -23.5502° |
| Constellation | Pyxis |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| TOI-6695 b | 80.4 days | 0.402 AU | 9.5276 R⊕ | 66.744 M⊕ | Transit, 2025 |
| TOI-6695 c | 242.4 days | 0.838 AU | 13.6 R⊕ estimated | 460.85 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 6,400 K, 3.5 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 1.71 to 2.97 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 922 years ago, around 1100.