TOI-5349 is 614 light-years from the Sun. The NASA Exoplanet Archive lists 1 planet around this M1+/-0.5 star; the first was found in 2026 by transit (Transiting Exoplanet Survey Satellite (TESS)).
Fly there in 3DTOI-5349 b goes round its star every 3.32 days, 27 times as often as Mercury goes round the Sun.
| Spectral type | M1+/-0.5 |
| Surface temperature | 3,751 K |
| Mass | 0.61 solar masses |
| Radius | 0.58 solar radii |
| Luminosity | 0.063 times the Sun |
| Apparent magnitude | 15.685 |
| Age | about 9 billion years |
| Distance from the Sun | 614.3 light-years (188.3 parsecs) |
| Position (J2000) | RA 52.7126°, Dec 20.8796° |
| Constellation | Taurus |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| TOI-5349 b | 3.32 days | 0.0369 AU | 10.2 R⊕ | 127.4 M⊕ | Transit, 2026 |
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 3,751 K, 0.063 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 0.26 to 0.50 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 614 years ago, around 1410.