Star · A7V
HIP 10795
HIP 10795 is a main-sequence star of spectral type A7V in the constellation Aries, 306.3 light-years from the Sun.
| Constellation | Aries |
|---|---|
| Distance | 306.3 light-years (93.9 pc) |
| Apparent magnitude | magnitude 6.45 |
| Absolute magnitude | magnitude 1.59 |
| Spectral type | A7V |
| Surface temperature | 7,010 K |
| Luminosity | 19.7 L☉ |
| Radius | 3.01 R☉ |
| Mass | 2.13 M☉ (estimated) |
| Right ascension (J2000) | 2h 18m 58.0s |
| Declination (J2000) | +23° 10′ 04″ |
| Space velocity (relative to the Sun) | 5.6 km/s |
In the sky
Visible to the naked eye under a dark sky (apparent magnitude 6.45). Visible from the whole Northern Hemisphere and south to latitude 67° S. North of latitude 67° N 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 1720. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 5.4 million years.
The Sun seen from there
From a planet around HIP 10795, the Sun would look like a star of magnitude 9.69, in the direction where our sky has the constellation Hydra. It would be invisible to the naked eye.
Neighbours
Its nearest neighbours in the catalogue (within 20 light-years):
- HIP 10201 16.7 light-years
Position, brightness and colour from the HYG / AT-HYG catalogue; temperature, luminosity, radius and mass are approximate values computed from these observations.