Star · F6IV
HIP 114725
HIP 114725 is a subgiant star of spectral type F6IV in the constellation Pegasus, 339.5 light-years from the Sun.
| Constellation | Pegasus |
|---|---|
| Distance | 339.5 light-years (104.1 pc) |
| Apparent magnitude | magnitude 6.41 |
| Absolute magnitude | magnitude 1.32 |
| Spectral type | F6IV |
| Surface temperature | 6,630 K |
| Luminosity | 25.2 L☉ |
| Radius | 3.8 R☉ |
| Mass | 2.28 M☉ (estimated) |
| Right ascension (J2000) | 23h 14m 21.7s |
| Declination (J2000) | +29° 46′ 19″ |
| Space velocity (relative to the Sun) | 16.3 km/s |
In the sky
Visible to the naked eye under a dark sky (apparent magnitude 6.41). Visible from the whole Northern Hemisphere and south to latitude 60° S. North of latitude 60° N it never sets. It stands highest at midnight in September, 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 114725, the Sun would look like a star of magnitude 9.92, in the direction where our sky has the constellation Hydra. 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.