Star · F9V
KIC 10525077
KIC 10525077 is a main-sequence star of spectral type F9V in the constellation Cygnus, 4,766 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).
| Constellation | Cygnus |
|---|---|
| Distance | 4,766 light-years (1,461 pc) |
| Apparent magnitude | magnitude 15.59 |
| Absolute magnitude | magnitude 4.77 |
| Spectral type | F9V |
| Surface temperature | 6,090 K |
| Luminosity | 1.35 L☉ |
| Radius | 1.01 R☉ |
| Mass | 1.01 M☉ |
| Metallicity [Fe/H] | -0.04 |
| Right ascension (J2000) | 19h 09m 30.7s |
| Declination (J2000) | +47° 46′ 16″ |
| Space velocity (relative to the Sun) | 29.8 km/s |
In the sky
A telescope is needed to see it: its apparent magnitude is 15.59. Visible from the whole Northern Hemisphere and south to latitude 42° S. North of latitude 42° 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 4,766 years ago. At that time the first farming villages were being founded; there was no writing yet. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 85 million years.
The Sun seen from there
From a planet around KIC 10525077, the Sun would look like a star of magnitude 15.65, in the direction where our sky has the constellation Puppis. It would be invisible to the naked eye.
Planets
- KIC 10525077 b 854-day orbit · 5.5 R⊕
Stellar parameters from the NASA Exoplanet Archive; position and brightness from the HYG / AT-HYG catalogue.