Star · F9V
Kepler-1915
Kepler-1915 is a main-sequence star of spectral type F9V in the constellation Cygnus, 4,940 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).
| Constellation | Cygnus |
|---|---|
| Distance | 4,940 light-years (1,515 pc) |
| Apparent magnitude | magnitude 16.26 |
| Absolute magnitude | magnitude 5.36 |
| Spectral type | F9V |
| Surface temperature | 6,020 K |
| Luminosity | 1.15 L☉ |
| Radius | 1.06 R☉ |
| Mass | 1.03 M☉ |
| Metallicity [Fe/H] | -0.06 |
| Right ascension (J2000) | 20h 05m 06.9s |
| Declination (J2000) | +44° 15′ 02″ |
| Space velocity (relative to the Sun) | 43.1 km/s |
In the sky
A telescope is needed to see it: its apparent magnitude is 16.26. Visible from the whole Northern Hemisphere and south to latitude 46° S. North of latitude 46° 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 4,940 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 88 million years.
The Sun seen from there
From a planet around Kepler-1915, the Sun would look like a star of magnitude 15.73, in the direction where our sky has the constellation Vela. It would be invisible to the naked eye.
Planets
- Kepler-1915 b 13.8-day orbit · 3.22 R⊕
Stellar parameters from the NASA Exoplanet Archive; position and brightness from the HYG / AT-HYG catalogue.