Kepler-880 is 1,961 light-years from the Sun. The NASA Exoplanet Archive lists 2 planets around this 6,761 K star; the first was found in 2016 by transit (Kepler).
Fly there in 3DKepler-880 b goes round its star every 7.71 days, 11 times as often as Mercury goes round the Sun.
| Surface temperature | 6,761 K |
| Mass | 1.46 solar masses |
| Radius | 1.74 solar radii |
| Luminosity | 4.635 times the Sun |
| Apparent magnitude | 11.845 |
| Age | about 1.66 billion years |
| Distance from the Sun | 1961.3 light-years (601.3 parsecs) |
| Position (J2000) | RA 281.9712°, Dec 43.6728° |
| Constellation | Lyra |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| Kepler-880 b | 7.71 days | 0.0915 AU | 2.66 R⊕ | 7.56 M⊕ estimated | Transit, 2016 |
| Kepler-880 c | 11.8 days | 0.122 AU | 2.87 R⊕ | 8.6 M⊕ estimated | Transit, 2023 |
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 6,761 K, 4.6 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 1.93 to 3.34 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 1,961 years ago, around AD 60.