Kepler-144 is 1,255 light-years from the Sun. The NASA Exoplanet Archive lists 2 planets around this 6,075 K star; the first was found in 2014 by transit (Kepler).
Fly there in 3DKepler-144 b goes round its star every 5.89 days, 15 times as often as Mercury goes round the Sun.
| Surface temperature | 6,075 K |
| Mass | 1.154 solar masses |
| Radius | 1.235 solar radii |
| Luminosity | 1.914 times the Sun |
| Apparent magnitude | 12.195 |
| Age | about 0.94 billion years |
| Distance from the Sun | 1255.4 light-years (384.9 parsecs) |
| Position (J2000) | RA 281.9156°, Dec 42.7756° |
| Constellation | Lyra |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| Kepler-144 b | 5.89 days | 0.0660 AU | 1.33 R⊕ | 2.33 M⊕ estimated | Transit, 2014 |
| Kepler-144 c | 10.1 days | 0.0940 AU | 1.35 R⊕ | 2.39 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 6,075 K, 1.9 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 1.29 to 2.26 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 1,255 years ago, around AD 770.