Star · K7V
Gl 910
Gl 910 is a main-sequence star of spectral type K7V in the constellation Pegasus, 64.9 light-years from the Sun.
| Other names | HIP 117779 |
|---|---|
| Constellation | Pegasus |
| Distance | 64.9 light-years (19.9 pc) |
| Apparent magnitude | magnitude 9.75 |
| Absolute magnitude | magnitude 8.25 |
| Spectral type | K7V |
| Surface temperature | 4,020 K |
| Luminosity | 0.119 L☉ |
| Radius | 0.711 R☉ |
| Mass | 0.588 M☉ (estimated) |
| Right ascension (J2000) | 23h 53m 08.6s |
| Declination (J2000) | +29° 01′ 05″ |
| Space velocity (relative to the Sun) | 7.8 km/s |
In the sky
A telescope is needed to see it: its apparent magnitude is 9.75. Visible from the whole Northern Hemisphere and south to latitude 61° S. North of latitude 61° 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 1961. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 1.2 million years.
The Sun seen from there
From a planet around Gl 910, the Sun would look like a star of magnitude 6.33, in the direction where our sky has the constellation Hydra. It would be visible to the naked eye.
Neighbours
Its nearest neighbours in the catalogue (within 20 light-years):
Position, brightness and colour from the HYG / AT-HYG catalogue; temperature, luminosity, radius and mass are approximate values computed from these observations.