Star · F7V
HIP 57587
HIP 57587 is a main-sequence star of spectral type F7V in the constellation Crater, 145.5 light-years from the Sun.
| Constellation | Crater |
|---|---|
| Distance | 145.5 light-years (44.6 pc) |
| Apparent magnitude | magnitude 6.24 |
| Absolute magnitude | magnitude 2.99 |
| Spectral type | F7V |
| Surface temperature | 6,030 K |
| Luminosity | 5.67 L☉ |
| Radius | 2.18 R☉ |
| Mass | 1.54 M☉ (estimated) |
| Right ascension (J2000) | 11h 48m 23.5s |
| Declination (J2000) | −10° 18′ 47″ |
| Space velocity (relative to the Sun) | 35.2 km/s |
In the sky
Visible to the naked eye under a dark sky (apparent magnitude 6.24). Visible from the whole Southern Hemisphere and north to latitude 80° N. South of latitude 80° S it never sets. It stands highest at midnight in March, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 1880. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 2.6 million years.
The Sun seen from there
From a planet around HIP 57587, the Sun would look like a star of magnitude 8.08, in the direction where our sky has the constellation Pegasus. 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.