Star · F3V
Kepler-507
Kepler-507 is a main-sequence star of spectral type F3V in the constellation Cygnus, 1,277 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).
| Constellation | Cygnus |
|---|---|
| Distance | 1,277 light-years (391.7 pc) |
| Apparent magnitude | magnitude 12.24 |
| Absolute magnitude | magnitude 4.28 |
| Spectral type | F3V |
| Surface temperature | 6,110 K |
| Luminosity | 2.12 L☉ |
| Radius | 1.32 R☉ |
| Mass | 1.16 M☉ |
| Age | 3.8 billion years |
| Metallicity [Fe/H] | 0.06 |
| Right ascension (J2000) | 19h 48m 04.5s |
| Declination (J2000) | +50° 24′ 32″ |
| Space velocity (relative to the Sun) | 22.8 km/s |
In the sky
A telescope is needed to see it: its apparent magnitude is 12.24. 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 749. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 23 million years.
The Sun seen from there
From a planet around Kepler-507, the Sun would look like a star of magnitude 12.79, in the direction where our sky has the constellation Puppis. It would be invisible to the naked eye.
Planets
- Kepler-507 b 3.57-day orbit · 1.3 R⊕
Stellar parameters from the NASA Exoplanet Archive; position and brightness from the HYG / AT-HYG catalogue.