Star · M0III
HIP 92630
HIP 92630 is a giant star of spectral type M0III in the constellation Telescopium, 811.8 light-years from the Sun.
| Constellation | Telescopium |
|---|---|
| Distance | 811.8 light-years (248.9 pc) |
| Apparent magnitude | magnitude 5.51 |
| Absolute magnitude | magnitude −1.47 |
| Spectral type | M0III |
| Surface temperature | 3,590 K |
| Luminosity | 1,630 L☉ |
| Radius | 104 R☉ |
| Mass | 7.52 M☉ (estimated) |
| Right ascension (J2000) | 18h 52m 27.2s |
| Declination (J2000) | −46° 35′ 42″ |
| Space velocity (relative to the Sun) | 42.6 km/s |
In the sky
Visible to the naked eye under a dark sky (apparent magnitude 5.51). Visible from the whole Southern Hemisphere and north to latitude 43° N. South of latitude 43° S it never sets. It stands highest at midnight in July, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 1214. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 14 million years.
The Sun seen from there
From a planet around HIP 92630, the Sun would look like a star of magnitude 11.81, in the direction where our sky has the constellation Auriga. 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.