Kepler-1464 is 3,756 light-years from the Sun. The NASA Exoplanet Archive lists 2 planets around this 5,828 K star; the first was found in 2016 by transit (Kepler).
Fly there in 3DKepler-1464 c goes round its star every 5.33 days, 17 times as often as Mercury goes round the Sun.
| Surface temperature | 5,828 K |
| Mass | 1.02 solar masses |
| Radius | 1.01 solar radii |
| Luminosity | 2.69 times the Sun |
| Apparent magnitude | 14.358 |
| Age | about 3.89 billion years |
| Distance from the Sun | 3756.4 light-years (1151.7 parsecs) |
| Position (J2000) | RA 287.2357°, Dec 38.7541° |
| Constellation | Lyra |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| Kepler-1464 c | 5.33 days | 0.0610 AU | 1 R⊕ | 0.972 M⊕ estimated | Transit, 2016 |
| Kepler-1464 b | 31.8 days | 0.201 AU | 1.66 R⊕ | 3.39 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 5,828 K, 2.7 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 1.55 to 2.74 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 3,756 years ago, around 1700 BC.