Kepler-529 is 2,606 light-years from the Sun. The NASA Exoplanet Archive lists 3 planets around this 6,087 K star; the first was found in 2016 by transit (Kepler).
Fly there in 3DKepler-529 b goes round its star every 47.5 hours, 44 times as often as Mercury goes round the Sun.
| Surface temperature | 6,087 K |
| Mass | 1.07 solar masses |
| Radius | 1.14 solar radii |
| Luminosity | 1.611 times the Sun |
| Apparent magnitude | 13.779 |
| Age | about 3.98 billion years |
| Distance from the Sun | 2606.0 light-years (799.0 parsecs) |
| Position (J2000) | RA 285.8884°, Dec 47.8804° |
| Constellation | Draco |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| Kepler-529 b | 47.5 hours | 0.0309 AU | 1.86 R⊕ | 4.12 M⊕ estimated | Transit, 2016 |
| Kepler-529 c | 12.8 days | 0.107 AU | 2 R⊕ | 4.66 M⊕ estimated | Transit, 2016 |
| Kepler-529 d | 35.9 days | 0.213 AU | 2.795 R⊕ | 8.22 M⊕ estimated | Transit, 2021 |
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 6,087 K, 1.6 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 1.18 to 2.07 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 2,606 years ago, around 600 BC.