TOI-5795 is 511 light-years from the Sun. The NASA Exoplanet Archive lists 1 planet around this G3 V star; the first was found in 2025 by transit (Transiting Exoplanet Survey Satellite (TESS)).
Fly there in 3DTOI-5795 b goes round its star every 6.14 days, 14 times as often as Mercury goes round the Sun.
| Spectral type | G3 V |
| Surface temperature | 5,715 K |
| Mass | 0.901 solar masses |
| Radius | 1.082 solar radii |
| Luminosity | 1.13 times the Sun |
| Apparent magnitude | 10.708 |
| Age | about 10.2 billion years |
| Distance from the Sun | 510.5 light-years (156.5 parsecs) |
| Position (J2000) | RA 304.8688°, Dec -7.5477° |
| Constellation | Aquila |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| TOI-5795 b | 6.14 days | 0.0640 AU | 5.62 R⊕ | 23.66 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 5,715 K, 1.1 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 1.01 to 1.79 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 1520.