Star · B9IV
11 Ari
11 Ari is a subgiant star of spectral type B9IV in the constellation Aries, 825.0 light-years from the Sun.
| Other names | HIP 9859 |
|---|---|
| Constellation | Aries |
| Distance | 825.0 light-years (252.9 pc) |
| Apparent magnitude | magnitude 6.01 |
| Absolute magnitude | magnitude −1.01 |
| Spectral type | B9IV |
| Surface temperature | 10,520 K |
| Luminosity | 323 L☉ |
| Radius | 5.41 R☉ |
| Mass | 4.73 M☉ (estimated) |
| Right ascension (J2000) | 2h 06m 49.2s |
| Declination (J2000) | +25° 42′ 16″ |
| Space velocity (relative to the Sun) | 28.4 km/s |
In the sky
Visible to the naked eye under a dark sky (apparent magnitude 6.01). Visible from the whole Northern Hemisphere and south to latitude 64° S. North of latitude 64° N it never sets. It stands highest at midnight in October, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 1201. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 15 million years.
The Sun seen from there
From a planet around 11 Ari, the Sun would look like a star of magnitude 11.85, in the direction where our sky has the constellation Hydra. 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.