Kepler-383 is 1,533 light-years from the Sun. The NASA Exoplanet Archive lists 2 planets around this 4,710 K star; the first was found in 2014 by transit (Kepler).
Fly there in 3DKepler-383 b goes round its star every 12.9 days, 7 times as often as Mercury goes round the Sun.
| Surface temperature | 4,710 K |
| Mass | 0.669 solar masses |
| Radius | 0.672 solar radii |
| Luminosity | 0.2004 times the Sun |
| Apparent magnitude | 15.473 |
| Age | about 13.9 billion years |
| Distance from the Sun | 1532.9 light-years (470.0 parsecs) |
| Position (J2000) | RA 291.3426°, Dec 38.3632° |
| Constellation | Lyra |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| Kepler-383 b | 12.9 days | 0.0950 AU | 1.32 R⊕ | 2.3 M⊕ estimated | Transit, 2014 |
| Kepler-383 c | 31.2 days | 0.172 AU | 1.24 R⊕ | 2.07 M⊕ estimated | 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 4,710 K, 0.20 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 0.45 to 0.82 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 1,533 years ago, around AD 490.