Star · B9IV
HIP 112508
HIP 112508 is a subgiant star of spectral type B9IV in the constellation Cepheus, 983.5 light-years from the Sun.
| Constellation | Cepheus |
|---|---|
| Distance | 983.5 light-years (301.5 pc) |
| Apparent magnitude | magnitude 6.33 |
| Absolute magnitude | magnitude −1.07 |
| Spectral type | B9IV |
| Surface temperature | 9,920 K |
| Luminosity | 311 L☉ |
| Radius | 5.97 R☉ |
| Mass | 4.68 M☉ (estimated) |
| Right ascension (J2000) | 22h 47m 23.2s |
| Declination (J2000) | +58° 28′ 59″ |
| Space velocity (relative to the Sun) | 15.7 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 32° S. North of latitude 32° N it never sets. It stands highest at midnight in August, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 1043. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 17 million years.
The Sun seen from there
From a planet around HIP 112508, the Sun would look like a star of magnitude 12.23, in the direction where our sky has the constellation Carina. 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.