TOI-1710 is 265 light-years from the Sun. The NASA Exoplanet Archive lists 1 planet around this G5 V star; the first was found in 2022 by transit (Transiting Exoplanet Survey Satellite (TESS)).
Fly there in 3DTOI-1710 b goes round its star every 24.3 days, 4 times as often as Mercury goes round the Sun.
TOI-1710 is one of 2 stars in its system: the other is drawn where the Washington Double Star Catalog measures it on the sky.
| Spectral type | G5 V |
| Surface temperature | 5,775 K |
| Mass | 1.02 solar masses |
| Radius | 0.93 solar radii |
| Luminosity | 0.86 times the Sun |
| Apparent magnitude | 9.545 |
| Age | about 1 billion years |
| Distance from the Sun | 264.9 light-years (81.2 parsecs) |
| Position (J2000) | RA 94.2838°, Dec 76.2110° |
| Constellation | Camelopardalis |
TOI-1710 B has no spectral type listed of magnitude 14.9, judged a true companion. In 2016 it was 44.5″ from TOI-1710, at position angle 203° (Washington Double Star Catalog, 06171+7613 UC 1419): 3,615 AU on the sky at this distance. The true distance can only be larger. Its colour is estimated from its brightness.
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| TOI-1710 b | 24.3 days | 0.165 AU | 5.06 R⊕ | 19.1 M⊕ | Transit, 2022 |
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 5,775 K, 0.86 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 0.88 to 1.55 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 265 years ago, around 1760.