Star · B9
HIP 84445
HIP 84445 is a main-sequence star of spectral type B9 in the constellation Scorpius, 346.2 light-years from the Sun.
| Constellation | Scorpius |
|---|---|
| Distance | 346.2 light-years (106.1 pc) |
| Apparent magnitude | magnitude 6.20 |
| Absolute magnitude | magnitude 1.07 |
| Spectral type | B9 |
| Surface temperature | 10,480 K |
| Luminosity | 47.4 L☉ |
| Radius | 2.09 R☉ |
| Mass | 2.74 M☉ (estimated) |
| Right ascension (J2000) | 17h 15m 51.4s |
| Declination (J2000) | −30° 12′ 39″ |
| Space velocity (relative to the Sun) | 24.0 km/s |
In the sky
Visible to the naked eye under a dark sky (apparent magnitude 6.20). Visible from the whole Southern Hemisphere and north to latitude 60° N. South of latitude 60° S it never sets. It stands highest at midnight in June, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 1680. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 6.1 million years.
The Sun seen from there
From a planet around HIP 84445, the Sun would look like a star of magnitude 9.96, in the direction where our sky has the constellation Auriga. 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.