Star · A8V
48 LMi
48 LMi is a main-sequence star of spectral type A8V in the constellation Leo Minor, 426.4 light-years from the Sun.
| Other names | HIP 53355 |
|---|---|
| Constellation | Leo Minor |
| Distance | 426.4 light-years (130.7 pc) |
| Apparent magnitude | magnitude 6.19 |
| Absolute magnitude | magnitude 0.61 |
| Spectral type | A8V |
| Surface temperature | 7,520 K |
| Luminosity | 49.6 L☉ |
| Radius | 4.15 R☉ |
| Mass | 2.77 M☉ (estimated) |
| Right ascension (J2000) | 10h 54m 42.2s |
| Declination (J2000) | +25° 29′ 27″ |
| Space velocity (relative to the Sun) | 37.8 km/s |
In the sky
Visible to the naked eye under a dark sky (apparent magnitude 6.19). Visible from the whole Northern Hemisphere and south to latitude 65° S. North of latitude 65° N 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 1600. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 7.6 million years.
The Sun seen from there
From a planet around 48 LMi, the Sun would look like a star of magnitude 10.41, in the direction where our sky has the constellation Piscis Austrinus. 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.