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Star · G2V

Gl 83.4B

Gl 83.4B is a main-sequence star of spectral type G2V in the constellation Phoenix, 163.5 light-years from the Sun.

ConstellationPhoenix
Distance163.5 light-years (50.1 pc)
Apparent magnitudemagnitude 11.50
Absolute magnitudemagnitude 8.00
Spectral typeG2V
Surface temperature5,780 K
Luminosity0.0586 L☉
Radius0.242 R☉
Mass0.492 M☉ (estimated)
Right ascension (J2000)2h 03m 54.9s
Declination (J2000)−45° 24′ 48″
Space velocity (relative to the Sun)75.1 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 11.50. Visible from the whole Southern Hemisphere and north to latitude 45° N. South of latitude 45° S it never sets. It stands highest at midnight in October, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1862. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 2.9 million years.

The Sun seen from there

From a planet around Gl 83.4B, the Sun would look like a star of magnitude 8.33, in the direction where our sky has the constellation Canes Venatici. It would be invisible to the naked eye.

Neighbours

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

  • Gl 83.4A 0.38 light-years
  • HIP 8232 10.7 light-years
  • HIP 8498 10.9 light-years
  • HIP 7858 15.8 light-years
  • HIP 10725 17.9 light-years
  • HIP 11989 18.5 light-years
  • HIP 7183 19.7 light-years
  • WISEA J013810.78-412220.2 19.9 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.