Kepler-324 is 1,636 light-years from the Sun. The NASA Exoplanet Archive lists 4 planets around this 5,194 K star; the first was found in 2014 by transit (Kepler).
Fly there in 3DKepler-324 b goes round its star every 4.39 days, 20 times as often as Mercury goes round the Sun.
| Surface temperature | 5,194 K |
| Mass | 0.901 solar masses |
| Radius | 0.84 solar radii |
| Luminosity | 0.4918 times the Sun |
| Apparent magnitude | 14.222 |
| Age | about 3.39 billion years |
| Distance from the Sun | 1635.9 light-years (501.6 parsecs) |
| Position (J2000) | RA 286.4714°, Dec 49.6491° |
| Constellation | Draco |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| Kepler-324 b | 4.39 days | 0.0500 AU | 1.14 R⊕ | 2414.4 M⊕ | Transit, 2014 |
| Kepler-324 e | 14.0 days | 0.110 AU | 2.0386 R⊕ | 235.01 M⊕ | Transit, 2021 |
| KOI-1831 d | 34.2 days | 0.199 AU | 1.13 R⊕ | 2.23 M⊕ | Transit, 2018 |
| Kepler-324 c | 51.8 days | 0.260 AU | 3.15 R⊕ | 6.2 M⊕ | 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 5,194 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 0.69 to 1.24 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 1,636 years ago, around AD 390.