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Star · G4V

Gl 10.1

Gl 10.1 is a main-sequence star of spectral type G4V in the constellation Tucana, 201.3 light-years from the Sun.

Other namesHIP 929
ConstellationTucana
Distance201.3 light-years (61.7 pc)
Apparent magnitudemagnitude 8.34
Absolute magnitudemagnitude 4.39
Spectral typeG4V
Surface temperature5,890 K
Luminosity1.6 L☉
Radius1.21 R☉
Mass1.12 M☉ (estimated)
Right ascension (J2000)0h 11m 33.1s
Declination (J2000)−58° 54′ 35″
Space velocity (relative to the Sun)79.4 km/s

In the sky

Too faint for the naked eye (magnitude 8.34); binoculars will find it. Visible from the whole Southern Hemisphere and north to latitude 31° N. South of latitude 31° S it never sets. It stands highest at midnight in September, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1825. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 3.6 million years.

The Sun seen from there

From a planet around Gl 10.1, the Sun would look like a star of magnitude 8.78, in the direction where our sky has the constellation Ursa Major. It would be invisible to the naked eye.

Neighbours

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

  • HIP 975 7.75 light-years
  • HIP 1582 13.7 light-years
  • HIP 1613 14.1 light-years
  • HIP 65 A 15.3 light-years
  • HIP 116710 15.3 light-years
  • HIP 2416 15.9 light-years
  • HIP 459 16.4 light-years
  • HIP 118092 17.0 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.