TOI-1695 is 147 light-years from the Sun. The NASA Exoplanet Archive lists 1 planet around this M1 V star; the first was found in 2022 by transit (Transiting Exoplanet Survey Satellite (TESS)).
Fly there in 3DTOI-1695 b goes round its star every 3.13 days, 28 times as often as Mercury goes round the Sun.
| Spectral type | M1 V |
| Surface temperature | 3,690 K |
| Mass | 0.513 solar masses |
| Radius | 0.515 solar radii |
| Luminosity | 0.0443 times the Sun |
| Apparent magnitude | 12.989 |
| Distance from the Sun | 147.2 light-years (45.1 parsecs) |
| Position (J2000) | RA 21.9217°, Dec 72.2966° |
| Constellation | Cassiopeia |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| TOI-1695 b | 3.13 days | 0.0335 AU | 1.9 R⊕ | 6.36 M⊕ | Transit, 2022 |
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 3,690 K, 0.044 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 0.22 to 0.42 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 147 years ago, around 1880.