Star · G
Kepler-1489
Kepler-1489 is a main-sequence star of spectral type G in the constellation Lyra, 4,185 light-years from the Sun. It is orbited by 2 confirmed exoplanet(s).
| Constellation | Lyra |
|---|---|
| Distance | 4,185 light-years (1,283 pc) |
| Apparent magnitude | magnitude 14.98 |
| Absolute magnitude | magnitude 4.44 |
| Spectral type | G |
| Surface temperature | 5,660 K |
| Luminosity | 1.58 L☉ |
| Radius | 0.9 R☉ |
| Mass | 0.93 M☉ |
| Age | 4.1 billion years |
| Metallicity [Fe/H] | -0.13 |
| Right ascension (J2000) | 18h 45m 11.0s |
| Declination (J2000) | +44° 27′ 55″ |
| Space velocity (relative to the Sun) | 21.9 km/s |
In the sky
A telescope is needed to see it: its apparent magnitude is 14.98. 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 June, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out 4,185 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 74 million years.
The Sun seen from there
From a planet around Kepler-1489, the Sun would look like a star of magnitude 15.37, in the direction where our sky has the constellation Puppis. It would be invisible to the naked eye.
Planets
- Kepler-1489 b 82.3-day orbit · 1.77 R⊕
- Kepler-1489 c 0.681-day orbit · 0.51 R⊕
Stellar parameters from the NASA Exoplanet Archive; position and brightness from the HYG / AT-HYG catalogue.