Kepler-1530 is 1,598 light-years from the Sun. The NASA Exoplanet Archive lists 3 planets around this 5,477 K star; the first was found in 2016 by transit (Kepler).
Fly there in 3DKepler-1530 b goes round its star every 2.59 days, 34 times as often as Mercury goes round the Sun.
| Surface temperature | 5,477 K |
| Mass | 0.92 solar masses |
| Radius | 0.88 solar radii |
| Luminosity | 0.4888 times the Sun |
| Apparent magnitude | 14.15 |
| Age | about 4.27 billion years |
| Distance from the Sun | 1597.8 light-years (489.9 parsecs) |
| Position (J2000) | RA 288.1624°, Dec 48.1652° |
| Constellation | Cygnus |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| Kepler-1530 b | 2.59 days | 0.0355 AU | 1.64 R⊕ | 3.33 M⊕ estimated | Transit, 2016 |
| Kepler-1530 c | 5.32 days | 0.0574 AU | 1.65 R⊕ | 3.36 M⊕ estimated | Transit, 2016 |
| Kepler-1530 d | 9.21 days | 0.0828 AU | 3.2787 R⊕ | 10.8 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 5,477 K, 0.49 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 0.68 to 1.20 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 1,598 years ago, around AD 430.