Star · K3V
Kepler-367
Kepler-367 is a main-sequence star of spectral type K3V in the constellation Cygnus, 613.3 light-years from the Sun. It is orbited by 2 confirmed exoplanet(s).
| Constellation | Cygnus |
|---|---|
| Distance | 613.3 light-years (188.0 pc) |
| Apparent magnitude | magnitude 13.19 |
| Absolute magnitude | magnitude 6.82 |
| Spectral type | K3V |
| Surface temperature | 4,710 K |
| Luminosity | 0.242 L☉ |
| Radius | 0.695 R☉ |
| Mass | 0.768 M☉ |
| Age | 2.3 billion years |
| Metallicity [Fe/H] | 0.20 |
| Right ascension (J2000) | 19h 49m 10.2s |
| Declination (J2000) | +49° 58′ 54″ |
| Space velocity (relative to the Sun) | 26.3 km/s |
In the sky
A telescope is needed to see it: its apparent magnitude is 13.19. Visible from the whole Northern Hemisphere and south to latitude 40° S. North of latitude 40° 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 the year 1413. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 11 million years.
The Sun seen from there
From a planet around Kepler-367, the Sun would look like a star of magnitude 11.20, in the direction where our sky has the constellation Puppis. It would be invisible to the naked eye.
Planets
- Kepler-367 b 37.8-day orbit · 1.3 R⊕
- Kepler-367 c 53.6-day orbit · 1.2 R⊕
Stellar parameters from the NASA Exoplanet Archive; position and brightness from the HYG / AT-HYG catalogue.