Kepler-323 is 1,484 light-years from the Sun. The NASA Exoplanet Archive lists 2 planets around this 6,004 K star; the first was found in 2014 by transit (Kepler).
Fly there in 3DKepler-323 b goes round its star every 40.3 hours, 52 times as often as Mercury goes round the Sun.
| Surface temperature | 6,004 K |
| Mass | 1.015 solar masses |
| Radius | 1.12 solar radii |
| Luminosity | 1.416 times the Sun |
| Apparent magnitude | 12.78 |
| Age | about 5.4 billion years |
| Distance from the Sun | 1483.6 light-years (454.9 parsecs) |
| Position (J2000) | RA 291.3823°, Dec 38.1275° |
| Constellation | Lyra |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| Kepler-323 b | 40.3 hours | 0.0278 AU | 1.381 R⊕ | 3.9 M⊕ | Transit, 2014 |
| Kepler-323 c | 3.55 days | 0.0458 AU | 1.57 R⊕ | 6.8 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 6,004 K, 1.4 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 1.12 to 1.96 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 1,484 years ago, around AD 540.