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Star · F2IV

Gl 391

Gl 391 is a subgiant star of spectral type F2IV in the constellation Carina, 53.1 light-years from the Sun.

Other namesHIP 50954
ConstellationCarina
Distance53.1 light-years (16.3 pc)
Apparent magnitudemagnitude 3.99
Absolute magnitudemagnitude 2.93
Spectral typeF2IV
Surface temperature7,050 K
Luminosity5.72 L☉
Radius1.6 R☉
Mass1.55 M☉ (estimated)
Right ascension (J2000)10h 24m 23.9s
Declination (J2000)−74° 01′ 54″
Space velocity (relative to the Sun)5.3 km/s

In the sky

Visible to the naked eye under a dark sky (apparent magnitude 3.99). Visible from the whole Southern Hemisphere and north to latitude 16° N. South of latitude 16° S 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 1973. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 942 thousand years.

The Sun seen from there

From a planet around Gl 391, the Sun would look like a star of magnitude 5.89, in the direction where our sky has the constellation Cepheus. 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.