Star · F5
HIP 95820
HIP 95820 is a supergiant star of spectral type F5 in the constellation Aquila, 1,885 light-years from the Sun.
| Constellation | Aquila |
|---|---|
| Distance | 1,885 light-years (578.0 pc) |
| Apparent magnitude | magnitude 6.37 |
| Absolute magnitude | magnitude −2.44 |
| Spectral type | F5 |
| Surface temperature | 5,080 K |
| Luminosity | 1,080 L☉ |
| Radius | 42.4 R☉ |
| Mass | 6.68 M☉ (estimated) |
| Right ascension (J2000) | 19h 29m 21.4s |
| Declination (J2000) | −7° 02′ 39″ |
| Space velocity (relative to the Sun) | 33.3 km/s |
In the sky
Visible to the naked eye under a dark sky (apparent magnitude 6.37). Visible from the whole Southern Hemisphere and north to latitude 83° N. 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 141. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 33 million years.
The Sun seen from there
From a planet around HIP 95820, the Sun would look like a star of magnitude 13.64, in the direction where our sky has the constellation Canis Minor. 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.