Kepler-1489 is 4,185 light-years from the Sun. The NASA Exoplanet Archive lists 2 planets around this G star; the first was found in 2016 by transit (Kepler).
Fly there in 3DKepler-1489 c goes round its star every 16.3 hours, 129 times as often as Mercury goes round the Sun.
Where the archive gives only a period or only an orbit size, the other is worked out from Kepler’s third law with the star’s mass.
| Spectral type | G |
| Surface temperature | 5,655 K |
| Mass | 0.93 solar masses |
| Radius | 0.9 solar radii |
| Luminosity | 1.576 times the Sun |
| Apparent magnitude | 14.983 |
| Age | about 4.07 billion years |
| Distance from the Sun | 4184.7 light-years (1283.0 parsecs) |
| Position (J2000) | RA 281.2958°, Dec 44.4654° |
| Constellation | Lyra |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| Kepler-1489 c | 16.3 hours | 0.0148 AU from Kepler’s law | 0.51 R⊕ | 0.087 M⊕ estimated | Transit, 2024 |
| Kepler-1489 b | 82.3 days | 0.368 AU | 1.77 R⊕ | 3.78 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.