Star · A0V
51 Aqr
51 Aqr is a main-sequence star of spectral type A0V in the constellation Aquarius, 405.7 light-years from the Sun.
| Other names | HIP 110578 |
|---|---|
| Constellation | Aquarius |
| Distance | 405.7 light-years (124.4 pc) |
| Apparent magnitude | magnitude 5.79 |
| Absolute magnitude | magnitude 0.32 |
| Spectral type | A0V |
| Surface temperature | 10,560 K |
| Luminosity | 96.2 L☉ |
| Radius | 2.93 R☉ |
| Mass | 3.35 M☉ (estimated) |
| Right ascension (J2000) | 22h 24m 06.9s |
| Declination (J2000) | −4° 50′ 13″ |
| Space velocity (relative to the Sun) | 17.5 km/s |
In the sky
Visible to the naked eye under a dark sky (apparent magnitude 5.79). Visible from the whole Southern Hemisphere and north to latitude 85° N. It stands highest at midnight in August, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 1620. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 7.2 million years.
The Sun seen from there
From a planet around 51 Aqr, the Sun would look like a star of magnitude 10.30, in the direction where our sky has the constellation Sextans. It would be invisible to the naked eye.
Position, brightness and colour from the HYG / AT-HYG catalogue; temperature, luminosity, radius and mass are approximate values computed from these observations.