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Star · G2V

Gl 838

Gl 838 is a main-sequence star of spectral type G2V in the constellation Grus, 50.7 light-years from the Sun.

Other namesHIP 107649
ConstellationGrus
Distance50.7 light-years (15.6 pc)
Apparent magnitudemagnitude 5.57
Absolute magnitudemagnitude 4.61
Spectral typeG2V
Surface temperature5,960 K
Luminosity1.29 L☉
Radius1.06 R☉
Mass1.07 M☉ (estimated)
Right ascension (J2000)21h 48m 15.8s
Declination (J2000)−47° 18′ 13″
Space velocity (relative to the Sun)26.0 km/s

In the sky

Visible to the naked eye under a dark sky (apparent magnitude 5.57). Visible from the whole Southern Hemisphere and north to latitude 43° N. South of latitude 43° S it never sets. It stands highest at midnight in August, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1975. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 900 thousand years.

The Sun seen from there

From a planet around Gl 838, the Sun would look like a star of magnitude 5.79, in the direction where our sky has the constellation Ursa Major. 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.