Star · M0V
HIP 24377
HIP 24377 is a main-sequence star of spectral type M0V in the constellation Orion, 1,108 light-years from the Sun.
| Constellation | Orion |
|---|---|
| Distance | 1,108 light-years (339.8 pc) |
| Apparent magnitude | magnitude 6.33 |
| Absolute magnitude | magnitude −1.33 |
| Spectral type | M0V |
| Surface temperature | 3,850 K |
| Luminosity | 992 L☉ |
| Radius | 70.8 R☉ |
| Mass | 6.52 M☉ (estimated) |
| Right ascension (J2000) | 5h 13m 47.3s |
| Declination (J2000) | +0° 33′ 38″ |
| Space velocity (relative to the Sun) | 33.6 km/s |
In the sky
Visible to the naked eye under a dark sky (apparent magnitude 6.33). Visible from the whole Northern Hemisphere and south to latitude 89° S. 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 918. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 20 million years.
The Sun seen from there
From a planet around HIP 24377, the Sun would look like a star of magnitude 12.49, 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.