Star · G8III
HIP 9095
HIP 9095 is a giant star of spectral type G8III in the constellation Phoenix, 217.0 light-years from the Sun.
| Constellation | Phoenix |
|---|---|
| Distance | 217.0 light-years (66.5 pc) |
| Apparent magnitude | magnitude 4.82 |
| Absolute magnitude | magnitude 0.70 |
| Spectral type | G8III |
| Surface temperature | 5,090 K |
| Luminosity | 59 L☉ |
| Radius | 9.86 R☉ |
| Mass | 2.91 M☉ (estimated) |
| Right ascension (J2000) | 1h 57m 10.1s |
| Declination (J2000) | −47° 23′ 07″ |
| Space velocity (relative to the Sun) | 36.0 km/s |
In the sky
Visible to the naked eye under a dark sky (apparent magnitude 4.82). 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 October, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 1809. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 3.8 million years.
The Sun seen from there
From a planet around HIP 9095, the Sun would look like a star of magnitude 8.95, in the direction where our sky has the constellation Canes Venatici. It would be invisible to the naked eye.
Neighbours
Its nearest neighbours in the catalogue (within 20 light-years):
- HIP 7579 15.4 light-years
- HIP 9495 16.8 light-years
- HIP 9672 17.2 light-years
Position, brightness and colour from the HYG / AT-HYG catalogue; temperature, luminosity, radius and mass are approximate values computed from these observations.