Star · K1IV
95 Cet
95 Cet is a subgiant star of spectral type K1IV in the constellation Cetus, 211.8 light-years from the Sun.
| Other names | HIP 15383 |
|---|---|
| Constellation | Cetus |
| Distance | 211.8 light-years (64.9 pc) |
| Apparent magnitude | magnitude 5.62 |
| Absolute magnitude | magnitude 1.56 |
| Spectral type | K1IV |
| Surface temperature | 4,630 K |
| Luminosity | 34.2 L☉ |
| Radius | 9.11 R☉ |
| Mass | 2.49 M☉ (estimated) |
| Right ascension (J2000) | 3h 18m 22.4s |
| Declination (J2000) | −0° 55′ 49″ |
| Space velocity (relative to the Sun) | 85.3 km/s |
In the sky
Visible to the naked eye under a dark sky (apparent magnitude 5.62). Visible from the whole Southern Hemisphere and north to latitude 89° N. It stands highest at midnight in November, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 1814. 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 95 Cet, the Sun would look like a star of magnitude 8.89, in the direction where our sky has the constellation Serpens. It would be invisible to the naked eye.
Neighbours
Its nearest neighbours in the catalogue (within 20 light-years):
- HIP 15812 12.4 light-years
- HIP 13957 18.4 light-years
Position, brightness and colour from the HYG / AT-HYG catalogue; temperature, luminosity, radius and mass are approximate values computed from these observations.