Star · B8V
Gomeisa
Gomeisa is a main-sequence star of spectral type B8V in the constellation Canis Minor, 161.7 light-years from the Sun.
| Other names | β CMi · HIP 36188 |
|---|---|
| Constellation | Canis Minor |
| Distance | 161.7 light-years (49.6 pc) |
| Apparent magnitude | magnitude 2.89 |
| Absolute magnitude | magnitude −0.59 |
| Spectral type | B8V |
| Surface temperature | 11,520 K |
| Luminosity | 259 L☉ |
| Radius | 4.04 R☉ |
| Mass | 4.44 M☉ (estimated) |
| Right ascension (J2000) | 7h 27m 09.0s |
| Declination (J2000) | +8° 17′ 22″ |
| Space velocity (relative to the Sun) | 26.7 km/s |
In the sky
Visible to the naked eye under a dark sky (apparent magnitude 2.89). Visible from the whole Northern Hemisphere and south to latitude 82° S. It stands highest at midnight in January, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 1864. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 2.9 million years.
The Sun seen from there
From a planet around Gomeisa, the Sun would look like a star of magnitude 8.31, in the direction where our sky has the constellation Aquila. It would be invisible to the naked eye.
Neighbours
Its nearest neighbours in the catalogue (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.