Star · G9 V
Kepler-67
Kepler-67 is a main-sequence star of spectral type G9 V in the constellation Cygnus, 3,689 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).
| Constellation | Cygnus |
|---|---|
| Distance | 3,689 light-years (1,131 pc) |
| Apparent magnitude | magnitude 16.17 |
| Absolute magnitude | magnitude 5.90 |
| Spectral type | G9 V |
| Surface temperature | 5,330 K |
| Luminosity | 0.42 L☉ |
| Radius | 0.778 R☉ |
| Mass | 0.865 M☉ |
| Age | 1.0 billion years |
| Metallicity [Fe/H] | -0.20 |
| Right ascension (J2000) | 19h 36m 36.8s |
| Declination (J2000) | +46° 09′ 59″ |
| Space velocity (relative to the Sun) | 50.0 km/s |
In the sky
A telescope is needed to see it: its apparent magnitude is 16.17. Visible from the whole Northern Hemisphere and south to latitude 44° S. North of latitude 44° N it never sets. It stands highest at midnight in July, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around 1664 BC. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 65 million years.
The Sun seen from there
From a planet around Kepler-67, the Sun would look like a star of magnitude 15.10, in the direction where our sky has the constellation Puppis. It would be invisible to the naked eye.
Planets
- Kepler-67 b 15.7-day orbit · 2.94 R⊕
Stellar parameters from the NASA Exoplanet Archive; position and brightness from the HYG / AT-HYG catalogue.