Star · G8IV
HIP 113852
HIP 113852 is a subgiant star of spectral type G8IV in the constellation Cassiopeia, 283.0 light-years from the Sun.
| Constellation | Cassiopeia |
|---|---|
| Distance | 283.0 light-years (86.8 pc) |
| Apparent magnitude | magnitude 6.43 |
| Absolute magnitude | magnitude 1.74 |
| Spectral type | G8IV |
| Surface temperature | 5,000 K |
| Luminosity | 23.7 L☉ |
| Radius | 6.48 R☉ |
| Mass | 2.24 M☉ (estimated) |
| Right ascension (J2000) | 23h 03m 21.4s |
| Declination (J2000) | +58° 33′ 50″ |
| Space velocity (relative to the Sun) | 26.2 km/s |
In the sky
Visible to the naked eye under a dark sky (apparent magnitude 6.43). Visible from the whole Northern Hemisphere and south to latitude 31° S. North of latitude 31° N it never sets. It stands highest at midnight in September, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 1743. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 5.0 million years.
The Sun seen from there
From a planet around HIP 113852, the Sun would look like a star of magnitude 9.52, in the direction where our sky has the constellation Carina. It would be invisible to the naked eye.
Neighbours
The catalogue has no other star within 20 light-years.
Position, brightness and colour from the HYG / AT-HYG catalogue; temperature, luminosity, radius and mass are approximate values computed from these observations.