Star · G8II
ε Sct
ε Sct is a bright giant star of spectral type G8II in the constellation Scutum, 571.2 light-years from the Sun.
| Other names | HIP 91845 |
|---|---|
| Constellation | Scutum |
| Distance | 571.2 light-years (175.1 pc) |
| Apparent magnitude | magnitude 4.88 |
| Absolute magnitude | magnitude −1.34 |
| Spectral type | G8II |
| Surface temperature | 4,490 K |
| Luminosity | 540 L☉ |
| Radius | 38.4 R☉ |
| Mass | 5.48 M☉ (estimated) |
| Right ascension (J2000) | 18h 43m 31.3s |
| Declination (J2000) | −8° 16′ 31″ |
| Space velocity (relative to the Sun) | 21.1 km/s |
In the sky
Visible to the naked eye under a dark sky (apparent magnitude 4.88). Visible from the whole Southern Hemisphere and north to latitude 82° N. It stands highest at midnight in June, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 1455. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 10 million years.
The Sun seen from there
From a planet around ε Sct, the Sun would look like a star of magnitude 11.05, in the direction where our sky has the constellation Monoceros. 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.