Star · A0V
HIP 62561
HIP 62561 is a main-sequence star of spectral type A0V in the constellation Camelopardalis, 406.4 light-years from the Sun.
| Constellation | Camelopardalis |
|---|---|
| Distance | 406.4 light-years (124.6 pc) |
| Apparent magnitude | magnitude 5.92 |
| Absolute magnitude | magnitude 0.44 |
| Spectral type | A0V |
| Surface temperature | 9,940 K |
| Luminosity | 77.7 L☉ |
| Radius | 2.97 R☉ |
| Mass | 3.15 M☉ (estimated) |
| Right ascension (J2000) | 12h 49m 06.7s |
| Declination (J2000) | +83° 25′ 04″ |
| Space velocity (relative to the Sun) | 17.9 km/s |
In the sky
Visible to the naked eye under a dark sky (apparent magnitude 5.92). Visible from the whole Northern Hemisphere and south to latitude 7° S. North of latitude 7° N it never sets.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 1620. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 7.2 million years.
The Sun seen from there
From a planet around HIP 62561, the Sun would look like a star of magnitude 10.31, in the direction where our sky has the constellation Octans. 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.