Star · A0V
HIP 60327
HIP 60327 is a main-sequence star of spectral type A0V in the constellation Coma Berenices, 338.9 light-years from the Sun.
| Constellation | Coma Berenices |
|---|---|
| Distance | 338.9 light-years (103.9 pc) |
| Apparent magnitude | magnitude 6.21 |
| Absolute magnitude | magnitude 1.13 |
| Spectral type | A0V |
| Surface temperature | 10,280 K |
| Luminosity | 43.6 L☉ |
| Radius | 2.08 R☉ |
| Mass | 2.67 M☉ (estimated) |
| Right ascension (J2000) | 12h 22m 10.8s |
| Declination (J2000) | +24° 46′ 26″ |
| Space velocity (relative to the Sun) | 28.6 km/s |
In the sky
Visible to the naked eye under a dark sky (apparent magnitude 6.21). Visible from the whole Northern Hemisphere and south to latitude 65° S. North of latitude 65° N 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 1687. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 6.0 million years.
The Sun seen from there
From a planet around HIP 60327, the Sun would look like a star of magnitude 9.91, in the direction where our sky has the constellation Cetus. 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.