Star · B3V
35 Ori
35 Ori is a main-sequence star of spectral type B3V in the constellation Orion, 1,076 light-years from the Sun.
| Other names | HIP 26093 |
|---|---|
| Constellation | Orion |
| Distance | 1,076 light-years (329.9 pc) |
| Apparent magnitude | magnitude 5.60 |
| Absolute magnitude | magnitude −1.99 |
| Spectral type | B3V |
| Surface temperature | 11,880 K |
| Luminosity | 1,000 L☉ |
| Radius | 7.47 R☉ |
| Mass | 6.54 M☉ (estimated) |
| Right ascension (J2000) | 5h 33m 54.3s |
| Declination (J2000) | +14° 18′ 20″ |
| Space velocity (relative to the Sun) | 20.3 km/s |
In the sky
Visible to the naked eye under a dark sky (apparent magnitude 5.60). Visible from the whole Northern Hemisphere and south to latitude 76° S. North of latitude 76° N it never sets. It stands highest at midnight in December, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 950. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 19 million years.
The Sun seen from there
From a planet around 35 Ori, the Sun would look like a star of magnitude 12.42, in the direction where our sky has the constellation Serpens. 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.