Kepler-352 is 824 light-years from the Sun. The NASA Exoplanet Archive lists 3 planets around this 5,212 K star; the first was found in 2014 by transit (Kepler).
Fly there in 3DKepler-352 d goes round its star every 6.89 days, 13 times as often as Mercury goes round the Sun.
| Surface temperature | 5,212 K |
| Mass | 0.798 solar masses |
| Radius | 0.781 solar radii |
| Luminosity | 0.3695 times the Sun |
| Apparent magnitude | 13.142 |
| Age | about 1.7 billion years |
| Distance from the Sun | 824.3 light-years (252.7 parsecs) |
| Position (J2000) | RA 299.8966°, Dec 46.0519° |
| Constellation | Cygnus |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| Kepler-352 d | 6.89 days | 0.0657 AU | 0.80628 R⊕ | 0.449 M⊕ estimated | Transit, 2021 |
| Kepler-352 b | 10.1 days | 0.0850 AU | 0.86 R⊕ | 0.566 M⊕ estimated | Transit, 2014 |
| Kepler-352 c | 16.3 days | 0.118 AU | 1.24 R⊕ | 2.07 M⊕ estimated | Transit, 2014 |
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 5,212 K, 0.37 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 0.60 to 1.07 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 824 years ago, around 1200.