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Star · G3V

Gl 379.2

Gl 379.2 is a main-sequence star of spectral type G3V in the constellation Antlia, 153.5 light-years from the Sun.

Other namesHIP 49793
ConstellationAntlia
Distance153.5 light-years (47.1 pc)
Apparent magnitudemagnitude 8.07
Absolute magnitudemagnitude 4.71
Spectral typeG3V
Surface temperature6,010 K
Luminosity1.17 L☉
Radius0.999 R☉
Mass1.04 M☉ (estimated)
Right ascension (J2000)10h 09m 49.6s
Declination (J2000)−36° 45′ 15″
Space velocity (relative to the Sun)155.5 km/s

In the sky

Too faint for the naked eye (magnitude 8.07); binoculars will find it. Visible from the whole Southern Hemisphere and north to latitude 53° N. South of latitude 53° 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 1873. 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 Gl 379.2, the Sun would look like a star of magnitude 8.19, in the direction where our sky has the constellation Lacerta. It would be invisible to the naked eye.

Neighbours

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

  • HIP 49599 3.76 light-years
  • HIP 50489 5.48 light-years
  • HIP 49024 5.74 light-years
  • HIP 48141 13.7 light-years
  • HIP 49767 15.6 light-years
  • HIP 49903 17.1 light-years
  • HIP 47251 17.3 light-years
  • HIP 47947 17.3 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.