Star · G8
HIP 35615
HIP 35615 is a supergiant star of spectral type G8 in the constellation Canis Major, 608.2 light-years from the Sun.
| Constellation | Canis Major |
|---|---|
| Distance | 608.2 light-years (186.5 pc) |
| Apparent magnitude | magnitude 5.59 |
| Absolute magnitude | magnitude −0.76 |
| Spectral type | G8 |
| Surface temperature | 4,810 K |
| Luminosity | 260 L☉ |
| Radius | 23.2 R☉ |
| Mass | 4.45 M☉ (estimated) |
| Right ascension (J2000) | 7h 20m 58.3s |
| Declination (J2000) | −14° 21′ 38″ |
| Space velocity (relative to the Sun) | 18.5 km/s |
In the sky
Visible to the naked eye under a dark sky (apparent magnitude 5.59). Visible from the whole Southern Hemisphere and north to latitude 76° N. South of latitude 76° S it never sets. It stands highest at midnight in January, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 1418. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 11 million years.
The Sun seen from there
From a planet around HIP 35615, the Sun would look like a star of magnitude 11.18, in the direction where our sky has the constellation Aquila. 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.