Star · A2IV
δ³ Tau
δ³ Tau is a subgiant star of spectral type A2IV in the constellation Taurus, 154.7 light-years from the Sun.
| Other names | HIP 20648 |
|---|---|
| Constellation | Taurus |
| Distance | 154.7 light-years (47.4 pc) |
| Apparent magnitude | magnitude 4.30 |
| Absolute magnitude | magnitude 0.92 |
| Spectral type | A2IV |
| Surface temperature | 9,550 K |
| Luminosity | 47.2 L☉ |
| Radius | 2.51 R☉ |
| Mass | 2.73 M☉ (estimated) |
| Right ascension (J2000) | 4h 25m 29.4s |
| Declination (J2000) | +17° 55′ 41″ |
| Space velocity (relative to the Sun) | 46.4 km/s |
In the sky
Visible to the naked eye under a dark sky (apparent magnitude 4.30). Visible from the whole Northern Hemisphere and south to latitude 72° S. North of latitude 72° N it never sets. It stands highest at midnight in November, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 1871. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 2.7 million years.
The Sun seen from there
From a planet around δ³ Tau, the Sun would look like a star of magnitude 8.21, in the direction where our sky has the constellation Ophiuchus. 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.