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Star · G8III

β LMi

β LMi is a giant star of spectral type G8III in the constellation Leo Minor, 153.9 light-years from the Sun.

Other namesHIP 51233
ConstellationLeo Minor
Distance153.9 light-years (47.2 pc)
Apparent magnitudemagnitude 4.20
Absolute magnitudemagnitude 0.83
Spectral typeG8III
Surface temperature4,980 K
Luminosity55.4 L☉
Radius10 R☉
Mass2.86 M☉ (estimated)
Right ascension (J2000)10h 27m 53.0s
Declination (J2000)+36° 42′ 26″
Space velocity (relative to the Sun)38.8 km/s

In the sky

Visible to the naked eye under a dark sky (apparent magnitude 4.20). Visible from the whole Northern Hemisphere and south to latitude 53° S. North of latitude 53° N it never sets. It stands highest at midnight in February, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1872. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 2.7 million years.

The Sun seen from there

From a planet around β LMi, the Sun would look like a star of magnitude 8.20, in the direction where our sky has the constellation Grus. It would be invisible to the naked eye.

Neighbours

Its nearest neighbours in the catalogue (within 20 light-years):

Open in the simulation

Position, brightness and colour from the HYG / AT-HYG catalogue; temperature, luminosity, radius and mass are approximate values computed from these observations.