TOI-4465 is 395 light-years from the Sun. The NASA Exoplanet Archive lists 1 planet around this G V star; the first was found in 2025 by transit (Transiting Exoplanet Survey Satellite (TESS)).
Fly there in 3DTOI-4465 b takes 101.9 days to go round its star once.
| Spectral type | G V |
| Surface temperature | 5,545 K |
| Mass | 0.93 solar masses |
| Radius | 1.014 solar radii |
| Luminosity | 0.8459 times the Sun |
| Apparent magnitude | 10.427 |
| Distance from the Sun | 395.1 light-years (121.1 parsecs) |
| Position (J2000) | RA 276.1340°, Dec 15.8419° |
| Constellation | Hercules |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| TOI-4465 b | 101.9 days | 0.416 AU | 14.011 R⊕ | 1872 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 5,545 K, 0.85 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 0.89 to 1.57 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 395 years ago, around 1630.