Kepler-453 is 1,444 light-years from the Sun. The NASA Exoplanet Archive lists 1 planet around this 5,527 K star; the first was found in 2015 by transit (Kepler).
Fly there in 3DKepler-453 b takes 240.5 days to go round its star once.
Kepler-453 is one of 2 stars in its system. The position of the other star is not catalogued, so only Kepler-453 and its planets are drawn.
| Surface temperature | 5,527 K |
| Mass | 0.944 solar masses |
| Radius | 0.833 solar radii |
| Luminosity | 0.6019 times the Sun |
| Apparent magnitude | 13.672 |
| Age | about 2.49 billion years |
| Distance from the Sun | 1444.4 light-years (442.9 parsecs) |
| Position (J2000) | RA 283.2413°, Dec 46.3785° |
| Constellation | Lyra |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| Kepler-453 b | 240.5 days | 0.790 AU | 6.204 R⊕ | 16 M⊕ | Transit, 2015 |
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 5,527 K, 0.60 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 0.75 to 1.33 AU. Its one known planet 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 1,444 years ago, around AD 580.