Star · B9V
HIP 76877
HIP 76877 is a main-sequence star of spectral type B9V in the constellation Apus, 417.4 light-years from the Sun.
| Constellation | Apus |
|---|---|
| Distance | 417.4 light-years (128.0 pc) |
| Apparent magnitude | magnitude 5.95 |
| Absolute magnitude | magnitude 0.41 |
| Spectral type | B9V |
| Surface temperature | 10,570 K |
| Luminosity | 88.1 L☉ |
| Radius | 2.8 R☉ |
| Mass | 3.27 M☉ (estimated) |
| Right ascension (J2000) | 15h 41m 54.7s |
| Declination (J2000) | −76° 04′ 55″ |
| Space velocity (relative to the Sun) | 26.4 km/s |
In the sky
Visible to the naked eye under a dark sky (apparent magnitude 5.95). Visible from the whole Southern Hemisphere and north to latitude 14° N. South of latitude 14° S it never sets.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 1609. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 7.4 million years.
The Sun seen from there
From a planet around HIP 76877, the Sun would look like a star of magnitude 10.37, in the direction where our sky has the constellation Camelopardalis. 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.