Star · K3I
HIP 30099
HIP 30099 is a supergiant star of spectral type K3I in the constellation Orion, 683.7 light-years from the Sun.
| Constellation | Orion |
|---|---|
| Distance | 683.7 light-years (209.6 pc) |
| Apparent magnitude | magnitude 5.67 |
| Absolute magnitude | magnitude −0.94 |
| Spectral type | K3I |
| Surface temperature | 3,680 K |
| Luminosity | 875 L☉ |
| Radius | 72.8 R☉ |
| Mass | 6.29 M☉ (estimated) |
| Right ascension (J2000) | 6h 20m 04.2s |
| Declination (J2000) | +14° 39′ 04″ |
| Space velocity (relative to the Sun) | 36.8 km/s |
In the sky
Visible to the naked eye under a dark sky (apparent magnitude 5.67). Visible from the whole Northern Hemisphere and south to latitude 75° S. North of latitude 75° N it never sets. It stands highest at midnight in December, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 1342. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 12 million years.
The Sun seen from there
From a planet around HIP 30099, the Sun would look like a star of magnitude 11.44, in the direction where our sky has the constellation Serpens. It would be invisible to the naked eye.
Position, brightness and colour from the HYG / AT-HYG catalogue; temperature, luminosity, radius and mass are approximate values computed from these observations.