Kepler-132 is 1,140 light-years from the Sun. The NASA Exoplanet Archive lists 4 planets around this 6,003 K star; the first was found in 2014 by transit (Kepler).
Fly there in 3DKepler-132 b goes round its star every 6.18 days, 14 times as often as Mercury goes round the Sun.
Kepler-132 is one of 2 stars in its system. The position of the other star is not catalogued, so only Kepler-132 and its planets are drawn.
| Surface temperature | 6,003 K |
| Mass | 0.929 solar masses |
| Radius | 1.178 solar radii |
| Luminosity | 1.626 times the Sun |
| Apparent magnitude | 11.922 |
| Age | about 4.37 billion years |
| Distance from the Sun | 1140.1 light-years (349.6 parsecs) |
| Position (J2000) | RA 283.2358°, Dec 41.3430° |
| Constellation | Lyra |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| Kepler-132 b | 6.18 days | 0.0670 AU | 1.21 R⊕ | 1.92 M⊕ estimated | Transit, 2014 |
| Kepler-132 c | 6.41 days | 0.0680 AU | 1.28 R⊕ | 2.18 M⊕ estimated | Transit, 2014 |
| Kepler-132 d | 18.0 days | 0.136 AU | 1.55 R⊕ | 3.02 M⊕ estimated | Transit, 2014 |
| Kepler-132 e | 110.3 days | 0.439 AU | 1.18 R⊕ | 1.76 M⊕ estimated | Transit, 2016 |
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 6,003 K, 1.6 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 1.20 to 2.10 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 1,140 years ago, around AD 890.