Star · F0V
51 Aql
51 Aql is a main-sequence star of spectral type F0V in the constellation Aquila, 89.6 light-years from the Sun.
| Other names | HIP 97650 |
|---|---|
| Constellation | Aquila |
| Distance | 89.6 light-years (27.5 pc) |
| Apparent magnitude | magnitude 5.38 |
| Absolute magnitude | magnitude 3.19 |
| Spectral type | F0V |
| Surface temperature | 6,870 K |
| Luminosity | 4.51 L☉ |
| Radius | 1.5 R☉ |
| Mass | 1.46 M☉ (estimated) |
| Right ascension (J2000) | 19h 50m 46.8s |
| Declination (J2000) | −10° 45′ 49″ |
| Space velocity (relative to the Sun) | 13.8 km/s |
In the sky
Visible to the naked eye under a dark sky (apparent magnitude 5.38). Visible from the whole Southern Hemisphere and north to latitude 79° N. South of latitude 79° S 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 1936. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 1.6 million years.
The Sun seen from there
From a planet around 51 Aql, the Sun would look like a star of magnitude 7.02, in the direction where our sky has the constellation Canis Minor. It would be invisible 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.