Star · M0
Gl 913
Gl 913 is a main-sequence star of spectral type M0 in the constellation Andromeda, 55.8 light-years from the Sun.
| Other names | HIP 118212 |
|---|---|
| Constellation | Andromeda |
| Distance | 55.8 light-years (17.1 pc) |
| Apparent magnitude | magnitude 9.57 |
| Absolute magnitude | magnitude 8.40 |
| Spectral type | M0 |
| Surface temperature | 4,030 K |
| Luminosity | 0.104 L☉ |
| Radius | 0.662 R☉ |
| Mass | 0.567 M☉ (estimated) |
| Right ascension (J2000) | 23h 58m 43.5s |
| Declination (J2000) | +46° 43′ 45″ |
| Space velocity (relative to the Sun) | 58.1 km/s |
In the sky
A telescope is needed to see it: its apparent magnitude is 9.57. Visible from the whole Northern Hemisphere and south to latitude 43° S. North of latitude 43° 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 1970. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 991 thousand years.
The Sun seen from there
From a planet around Gl 913, the Sun would look like a star of magnitude 6.00, in the direction where our sky has the constellation Centaurus. 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.