Kepler-1834 is 1,632 light-years from the Sun. The NASA Exoplanet Archive lists 2 planets around this 4,821 K star; the first was found in 2021 by transit (Kepler).
Fly there in 3DKepler-1834 c goes round its star every 18.4 hours, 115 times as often as Mercury goes round the Sun.
| Surface temperature | 4,821 K |
| Mass | 0.765 solar masses |
| Radius | 0.788 solar radii |
| Luminosity | 0.2651 times the Sun |
| Apparent magnitude | 15.18 |
| Age | about 12.2 billion years |
| Distance from the Sun | 1632.1 light-years (500.4 parsecs) |
| Position (J2000) | RA 294.6647°, Dec 39.7838° |
| Constellation | Cygnus |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| Kepler-1834 c | 18.4 hours | 0.0150 AU | 1.22 R⊕ | 1.98 M⊕ estimated | Transit, 2023 |
| Kepler-1834 b | 4.60 days | 0.0491 AU | 1.4594 R⊕ | 2.73 M⊕ estimated | Transit, 2021 |
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 4,821 K, 0.27 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 0.52 to 0.94 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 1,632 years ago, around AD 390.