Kepler-202 is 930 light-years from the Sun. The NASA Exoplanet Archive lists 2 planets around this 4,668 K star; the first was found in 2014 by transit (Kepler).
Fly there in 3DKepler-202 b goes round its star every 4.07 days, 22 times as often as Mercury goes round the Sun.
| Surface temperature | 4,668 K |
| Mass | 0.683 solar masses |
| Radius | 0.667 solar radii |
| Luminosity | 0.2301 times the Sun |
| Apparent magnitude | 14.178 |
| Age | about 3.24 billion years |
| Distance from the Sun | 929.9 light-years (285.1 parsecs) |
| Position (J2000) | RA 282.9735°, Dec 41.3218° |
| Constellation | Lyra |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| Kepler-202 b | 4.07 days | 0.0450 AU | 1.63 R⊕ | 3.29 M⊕ estimated | Transit, 2014 |
| Kepler-202 c | 16.3 days | 0.113 AU | 1.85 R⊕ | 4.08 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 4,668 K, 0.23 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 0.48 to 0.89 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 930 years ago, around 1100.