TOI-1807 is 139 light-years from the Sun. The NASA Exoplanet Archive lists 1 planet around this 4,914 K star; the first was found in 2021 by transit (Transiting Exoplanet Survey Satellite (TESS)).
Fly there in 3DTOI-1807 b goes round its star every 13.2 hours, 160 times as often as Mercury goes round the Sun.
| Surface temperature | 4,914 K |
| Mass | 0.8048 solar masses |
| Radius | 0.746 solar radii |
| Luminosity | 0.293 times the Sun |
| Apparent magnitude | 10 |
| Age | about 2.1 billion years |
| Distance from the Sun | 138.9 light-years (42.6 parsecs) |
| Position (J2000) | RA 201.2826°, Dec 38.9224° |
| Constellation | Canes Venatici |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| TOI-1807 b | 13.2 hours | 0.0122 AU | 1.4968 R⊕ | 2.44 M⊕ | Transit, 2021 |
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 4,914 K, 0.29 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 0.54 to 0.98 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 139 years ago, around 1890.