Star · B3V
HIP 35611
HIP 35611 is a main-sequence star of spectral type B3V in the constellation Canis Major, 2,119 light-years from the Sun.
| Constellation | Canis Major |
|---|---|
| Distance | 2,119 light-years (649.7 pc) |
| Apparent magnitude | magnitude 6.00 |
| Absolute magnitude | magnitude −3.06 |
| Spectral type | B3V |
| Surface temperature | 12,950 K |
| Luminosity | 3,200 L☉ |
| Radius | 11.2 R☉ |
| Mass | 9.12 M☉ (estimated) |
| Right ascension (J2000) | 7h 20m 54.9s |
| Declination (J2000) | −26° 57′ 50″ |
| Space velocity (relative to the Sun) | 28.5 km/s |
In the sky
Visible to the naked eye under a dark sky (apparent magnitude 6.00). Visible from the whole Southern Hemisphere and north to latitude 63° N. South of latitude 63° 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 94 BC. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 38 million years.
The Sun seen from there
From a planet around HIP 35611, the Sun would look like a star of magnitude 13.89, in the direction where our sky has the constellation Vulpecula. 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.