Star · K5V
Gl 415
Gl 415 is a main-sequence star of spectral type K5V in the constellation Crater, 64.8 light-years from the Sun.
| Other names | HIP 54651 |
|---|---|
| Constellation | Crater |
| Distance | 64.8 light-years (19.9 pc) |
| Apparent magnitude | magnitude 9.23 |
| Absolute magnitude | magnitude 7.74 |
| Spectral type | K5V |
| Surface temperature | 4,550 K |
| Luminosity | 0.121 L☉ |
| Radius | 0.56 R☉ |
| Mass | 0.59 M☉ (estimated) |
| Right ascension (J2000) | 11h 11m 10.7s |
| Declination (J2000) | −10° 57′ 03″ |
| Space velocity (relative to the Sun) | 111.4 km/s |
In the sky
A telescope is needed to see it: its apparent magnitude is 9.23. Visible from the whole Southern Hemisphere and north to latitude 79° N. South of latitude 79° S it never sets. It stands highest at midnight in March, 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 415, the Sun would look like a star of magnitude 6.32, in the direction where our sky has the constellation Pegasus. 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.