Star · F7V
HIP 91880
HIP 91880 is a main-sequence star of spectral type F7V in the constellation Scutum, 236.7 light-years from the Sun.
| Constellation | Scutum |
|---|---|
| Distance | 236.7 light-years (72.6 pc) |
| Apparent magnitude | magnitude 6.30 |
| Absolute magnitude | magnitude 2.00 |
| Spectral type | F7V |
| Surface temperature | 6,490 K |
| Luminosity | 13.6 L☉ |
| Radius | 2.92 R☉ |
| Mass | 1.92 M☉ (estimated) |
| Right ascension (J2000) | 18h 43m 51.2s |
| Declination (J2000) | −6° 49′ 05″ |
| Space velocity (relative to the Sun) | 68.6 km/s |
In the sky
Visible to the naked eye under a dark sky (apparent magnitude 6.30). Visible from the whole Southern Hemisphere and north to latitude 83° 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 1789. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 4.2 million years.
The Sun seen from there
From a planet around HIP 91880, the Sun would look like a star of magnitude 9.13, in the direction where our sky has the constellation Monoceros. It would be invisible to the naked eye.
Neighbours
Its nearest neighbours in the catalogue (within 20 light-years):
- HIP 92589 14.0 light-years
- HIP 92781 14.5 light-years
- HIP 91751 16.1 light-years
Position, brightness and colour from the HYG / AT-HYG catalogue; temperature, luminosity, radius and mass are approximate values computed from these observations.