Star · K0III
HIP 67250
HIP 67250 is a giant star of spectral type K0III in the constellation Canes Venatici, 299.0 light-years from the Sun.
| Constellation | Canes Venatici |
|---|---|
| Distance | 299.0 light-years (91.7 pc) |
| Apparent magnitude | magnitude 5.51 |
| Absolute magnitude | magnitude 0.70 |
| Spectral type | K0III |
| Surface temperature | 4,660 K |
| Luminosity | 74 L☉ |
| Radius | 13.2 R☉ |
| Mass | 3.11 M☉ (estimated) |
| Right ascension (J2000) | 13h 46m 59.8s |
| Declination (J2000) | +38° 32′ 34″ |
| Space velocity (relative to the Sun) | 60.2 km/s |
In the sky
Visible to the naked eye under a dark sky (apparent magnitude 5.51). Visible from the whole Northern Hemisphere and south to latitude 51° S. North of latitude 51° N it never sets. It stands highest at midnight in April, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 1727. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 5.3 million years.
The Sun seen from there
From a planet around HIP 67250, the Sun would look like a star of magnitude 9.64, in the direction where our sky has the constellation Fornax. It would be invisible to the naked eye.
Neighbours
Its nearest neighbours in the catalogue (within 20 light-years):
- HIP 67041 10.4 light-years
- HIP 68461 18.5 light-years
- SDSS J140409.91+400214.0 19.6 light-years
Position, brightness and colour from the HYG / AT-HYG catalogue; temperature, luminosity, radius and mass are approximate values computed from these observations.