TOI-2449 is 511 light-years from the Sun. The NASA Exoplanet Archive lists 1 planet around this G star; the first was found in 2025 by transit (Transiting Exoplanet Survey Satellite (TESS)).
Fly there in 3DTOI-2449 b takes 106.1 days to go round its star once.
| Spectral type | G |
| Surface temperature | 6,021 K |
| Mass | 1.079 solar masses |
| Radius | 1.065 solar radii |
| Luminosity | 1.406 times the Sun |
| Apparent magnitude | 10.416 |
| Age | about 2.5 billion years |
| Distance from the Sun | 511.4 light-years (156.8 parsecs) |
| Position (J2000) | RA 67.9844°, Dec -34.4555° |
| Constellation | Eridanus |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| TOI-2449 b | 106.1 days | 0.450 AU | 11.24 R⊕ | 222 M⊕ | Transit, 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 6,021 K, 1.4 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 1.11 to 1.95 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 511 years ago, around 1510.