Kepler-1052 is 3,077 light-years from the Sun. The NASA Exoplanet Archive lists 2 planets around this 5,888 K star; the first was found in 2016 by transit (Kepler).
Fly there in 3DKepler-1052 b goes round its star every 34.9 days, 2.5 times as often as Mercury goes round the Sun.
| Surface temperature | 5,888 K |
| Mass | 1.03 solar masses |
| Radius | 1.03 solar radii |
| Luminosity | 0.8977 times the Sun |
| Apparent magnitude | 14.932 |
| Age | about 3.55 billion years |
| Distance from the Sun | 3077.1 light-years (943.4 parsecs) |
| Position (J2000) | RA 295.3427°, Dec 46.6022° |
| Constellation | Cygnus |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| Kepler-1052 b | 34.9 days | 0.210 AU | 2.93 R⊕ | 8.91 M⊕ estimated | Transit, 2016 |
| Kepler-1052 c | 180.9 days | 0.614 AU | 2.3 R⊕ | 5.9 M⊕ estimated | Transit, 2023 |
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 5,888 K, 0.90 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 3,077 years ago, around 1100 BC.