Star · K5III
HIP 69462
HIP 69462 is a giant star of spectral type K5III in the constellation Centaurus, 1,476 light-years from the Sun.
| Constellation | Centaurus |
|---|---|
| Distance | 1,476 light-years (452.7 pc) |
| Apparent magnitude | magnitude 5.53 |
| Absolute magnitude | magnitude −2.75 |
| Spectral type | K5III |
| Surface temperature | 3,890 K |
| Luminosity | 3,500 L☉ |
| Radius | 130 R☉ |
| Mass | 9.35 M☉ (estimated) |
| Right ascension (J2000) | 14h 13m 16.4s |
| Declination (J2000) | −53° 39′ 56″ |
| Space velocity (relative to the Sun) | 36.9 km/s |
In the sky
Visible to the naked eye under a dark sky (apparent magnitude 5.53). Visible from the whole Southern Hemisphere and north to latitude 36° N. South of latitude 36° S it never sets. It stands highest at midnight in April, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 550. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 26 million years.
The Sun seen from there
From a planet around HIP 69462, the Sun would look like a star of magnitude 13.11, 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.