TOI-1749 is 325 light-years from the Sun. The NASA Exoplanet Archive lists 3 planets around this M0 V star; the first was found in 2021 by transit (Transiting Exoplanet Survey Satellite (TESS)).
Fly there in 3DTOI-1749 b goes round its star every 2.39 days, 37 times as often as Mercury goes round the Sun.
| Spectral type | M0 V |
| Surface temperature | 3,985 K |
| Mass | 0.58 solar masses |
| Radius | 0.55 solar radii |
| Luminosity | 0.06974 times the Sun |
| Apparent magnitude | 13.86 |
| Age | about 0.8 billion years |
| Distance from the Sun | 324.7 light-years (99.6 parsecs) |
| Position (J2000) | RA 282.7372°, Dec 64.4195° |
| Constellation | Draco |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| TOI-1749 b | 2.39 days | 0.0291 AU | 1.39 R⊕ | 57 M⊕ | Transit, 2021 |
| TOI-1749 c | 4.49 days | 0.0443 AU | 2.12 R⊕ | 14 M⊕ | Transit, 2021 |
| TOI-1749 d | 9.05 days | 0.0707 AU | 2.52 R⊕ | 15 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 3,985 K, 0.070 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 0.27 to 0.51 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 325 years ago, around 1700.