Star · G8V
ξ Boo
ξ Boo is a main-sequence star of spectral type G8V in the constellation Boötes, 22.0 light-years from the Sun.
| Other names | Gl 566A · HIP 72659 |
|---|---|
| Constellation | Boötes |
| Distance | 22.0 light-years (6.75 pc) |
| Apparent magnitude | magnitude 4.54 |
| Absolute magnitude | magnitude 5.39 |
| Spectral type | G8V |
| Surface temperature | 5,530 K |
| Luminosity | 0.682 L☉ |
| Radius | 0.898 R☉ |
| Mass | 0.909 M☉ (estimated) |
| Right ascension (J2000) | 14h 51m 23.4s |
| Declination (J2000) | +19° 06′ 01″ |
| Space velocity (relative to the Sun) | 4.6 km/s |
In the sky
Visible to the naked eye under a dark sky (apparent magnitude 4.54). Visible from the whole Northern Hemisphere and south to latitude 71° S. North of latitude 71° N it never sets. It stands highest at midnight in May, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 2004. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 391 thousand years.
The Sun seen from there
From a planet around ξ Boo, the Sun would look like a star of magnitude 3.98, in the direction where our sky has the constellation Eridanus. It would be visible to the naked eye.
Neighbours
Its nearest neighbours in the catalogue (within 20 light-years):
Position, brightness and colour from the HYG / AT-HYG catalogue; temperature, luminosity, radius and mass are approximate values computed from these observations.