Star · A4V
HIP 27341
HIP 27341 is a main-sequence star of spectral type A4V in the constellation Orion, 1,285 light-years from the Sun.
| Constellation | Orion |
|---|---|
| Distance | 1,285 light-years (394.0 pc) |
| Apparent magnitude | magnitude 6.04 |
| Absolute magnitude | magnitude −1.94 |
| Spectral type | A4V |
| Surface temperature | 8,700 K |
| Luminosity | 582 L☉ |
| Radius | 10.6 R☉ |
| Mass | 5.6 M☉ (estimated) |
| Right ascension (J2000) | 5h 47m 26.9s |
| Declination (J2000) | −10° 31′ 59″ |
| Space velocity (relative to the Sun) | 32.9 km/s |
In the sky
Visible to the naked eye under a dark sky (apparent magnitude 6.04). Visible from the whole Southern Hemisphere and north to latitude 79° N. South of latitude 79° S it never sets. It stands highest at midnight in December, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 741. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 23 million years.
The Sun seen from there
From a planet around HIP 27341, the Sun would look like a star of magnitude 12.81, in the direction where our sky has the constellation Ophiuchus. 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.