Kepler-184 is 1,991 light-years from the Sun. The NASA Exoplanet Archive lists 3 planets around this 5,788 K star; the first was found in 2014 by transit (Kepler).
Fly there in 3DKepler-184 b goes round its star every 10.7 days, 8 times as often as Mercury goes round the Sun.
| Surface temperature | 5,788 K |
| Mass | 0.872 solar masses |
| Radius | 0.873 solar radii |
| Luminosity | 0.5955 times the Sun |
| Apparent magnitude | 14.42 |
| Age | about 2.95 billion years |
| Distance from the Sun | 1990.6 light-years (610.3 parsecs) |
| Position (J2000) | RA 291.9519°, Dec 43.0746° |
| Constellation | Lyra |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| Kepler-184 b | 10.7 days | 0.0920 AU | 2.36 R⊕ | 6.17 M⊕ estimated | Transit, 2014 |
| Kepler-184 c | 20.3 days | 0.141 AU | 1.97 R⊕ | 8.8 M⊕ | Transit, 2014 |
| Kepler-184 d | 29.0 days | 0.179 AU | 2.49 R⊕ | 6.76 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 5,788 K, 0.60 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 0.73 to 1.29 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 1,991 years ago, around AD 40.