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Star · K8V

Gl 380

Gl 380 is a main-sequence star of spectral type K8V in the constellation Ursa Major, 15.9 light-years from the Sun.

Other namesHIP 49908
ConstellationUrsa Major
Distance15.9 light-years (4.87 pc)
Apparent magnitudemagnitude 6.60
Absolute magnitudemagnitude 8.16
Spectral typeK8V
Surface temperature4,080 K
Luminosity0.123 L☉
Radius0.703 R☉
Mass0.592 M☉ (estimated)
Right ascension (J2000)10h 11m 22.0s
Declination (J2000)+49° 27′ 15″
Space velocity (relative to the Sun)42.7 km/s

In the sky

Too faint for the naked eye (magnitude 6.60); binoculars will find it. Visible from the whole Northern Hemisphere and south to latitude 41° S. North of latitude 41° 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 2010. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 282 thousand years.

The Sun seen from there

From a planet around Gl 380, the Sun would look like a star of magnitude 3.27, in the direction where our sky has the constellation Grus. It would be visible 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.