Star · B8V
HIP 79199
HIP 79199 is a main-sequence star of spectral type B8V in the constellation Scorpius, 401.9 light-years from the Sun.
| Constellation | Scorpius |
|---|---|
| Distance | 401.9 light-years (123.2 pc) |
| Apparent magnitude | magnitude 5.50 |
| Absolute magnitude | magnitude 0.05 |
| Spectral type | B8V |
| Surface temperature | 11,170 K |
| Luminosity | 136 L☉ |
| Radius | 3.12 R☉ |
| Mass | 3.7 M☉ (estimated) |
| Right ascension (J2000) | 16h 09m 52.6s |
| Declination (J2000) | −33° 32′ 45″ |
| Space velocity (relative to the Sun) | 30.5 km/s |
In the sky
Visible to the naked eye under a dark sky (apparent magnitude 5.50). Visible from the whole Southern Hemisphere and north to latitude 56° N. South of latitude 56° S 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 1624. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 7.1 million years.
The Sun seen from there
From a planet around HIP 79199, the Sun would look like a star of magnitude 10.28, in the direction where our sky has the constellation Perseus. 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.