Star · A8IV
η Ant
η Ant is a subgiant star of spectral type A8IV in the constellation Antlia, 108.5 light-years from the Sun.
| Other names | HIP 48926 |
|---|---|
| Constellation | Antlia |
| Distance | 108.5 light-years (33.3 pc) |
| Apparent magnitude | magnitude 5.23 |
| Absolute magnitude | magnitude 2.62 |
| Spectral type | A8IV |
| Surface temperature | 7,460 K |
| Luminosity | 7.76 L☉ |
| Radius | 1.67 R☉ |
| Mass | 1.67 M☉ (estimated) |
| Right ascension (J2000) | 9h 58m 52.3s |
| Declination (J2000) | −35° 53′ 28″ |
| Space velocity (relative to the Sun) | 28.3 km/s |
In the sky
Visible to the naked eye under a dark sky (apparent magnitude 5.23). Visible from the whole Southern Hemisphere and north to latitude 54° N. South of latitude 54° S it never sets. It stands highest at midnight in February, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 1917. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 1.9 million years.
The Sun seen from there
From a planet around η Ant, the Sun would look like a star of magnitude 7.44, in the direction where our sky has the constellation Pegasus. It would be invisible 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.