TOI-1472 is 397 light-years from the Sun. The NASA Exoplanet Archive lists 2 planets around this 5,100 K star; the first was found in 2024 by transit (Transiting Exoplanet Survey Satellite (TESS)).
Fly there in 3DTOI-1472 b goes round its star every 6.36 days, 14 times as often as Mercury goes round the Sun.
| Surface temperature | 5,100 K |
| Mass | 0.87 solar masses |
| Radius | 0.84 solar radii |
| Luminosity | 0.441 times the Sun |
| Apparent magnitude | 11.302 |
| Age | about 3.1 billion years |
| Distance from the Sun | 397.4 light-years (121.8 parsecs) |
| Position (J2000) | RA 14.1143°, Dec 48.6375° |
| Constellation | Cassiopeia |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| TOI-1472 b | 6.36 days | 0.0640 AU | 4.058 R⊕ | 18.05 M⊕ | Transit, 2024 |
| TOI-1472 c | 15.5 days | 0.116 AU | 3.334 R⊕ | 21.13 M⊕ | 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 5,100 K, 0.44 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 0.66 to 1.18 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 397 years ago, around 1630.