Star · K9V
Kepler-1628
Kepler-1628 is a main-sequence star of spectral type K9V in the constellation Lyra, 1,148 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).
| Constellation | Lyra |
|---|---|
| Distance | 1,148 light-years (352.0 pc) |
| Apparent magnitude | magnitude 17.83 |
| Absolute magnitude | magnitude 10.10 |
| Spectral type | K9V |
| Surface temperature | 3,720 K |
| Luminosity | 0.0468 L☉ |
| Radius | 0.52 R☉ |
| Mass | 0.55 M☉ |
| Age | 5.1 billion years |
| Metallicity [Fe/H] | 0.17 |
| Right ascension (J2000) | 18h 46m 32.1s |
| Declination (J2000) | +43° 24′ 42″ |
| Space velocity (relative to the Sun) | 21.2 km/s |
In the sky
A telescope is needed to see it: its apparent magnitude is 17.83. Visible from the whole Northern Hemisphere and south to latitude 47° S. North of latitude 47° 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 878. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 20 million years.
The Sun seen from there
From a planet around Kepler-1628, the Sun would look like a star of magnitude 12.56, in the direction where our sky has the constellation Puppis. It would be invisible to the naked eye.
Planets
- Kepler-1628 b 76.4-day orbit · 6.43 R⊕
Stellar parameters from the NASA Exoplanet Archive; position and brightness from the HYG / AT-HYG catalogue.