Star · B3V
HIP 62327
HIP 62327 is a main-sequence star of spectral type B3V in the constellation Crux, 335.1 light-years from the Sun.
| Constellation | Crux |
|---|---|
| Distance | 335.1 light-years (102.7 pc) |
| Apparent magnitude | magnitude 4.62 |
| Absolute magnitude | magnitude −0.44 |
| Spectral type | B3V |
| Surface temperature | 12,490 K |
| Luminosity | 265 L☉ |
| Radius | 3.48 R☉ |
| Mass | 4.47 M☉ (estimated) |
| Right ascension (J2000) | 12h 46m 22.7s |
| Declination (J2000) | −56° 29′ 20″ |
| Space velocity (relative to the Sun) | 24.7 km/s |
In the sky
Visible to the naked eye under a dark sky (apparent magnitude 4.62). Visible from the whole Southern Hemisphere and north to latitude 34° N. South of latitude 34° S it never sets. It stands highest at midnight in March, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 1691. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 5.9 million years.
The Sun seen from there
From a planet around HIP 62327, the Sun would look like a star of magnitude 9.89, in the direction where our sky has the constellation Cassiopeia. 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.