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Star · A2V

τ Cen

τ Cen is a main-sequence star of spectral type A2V in the constellation Centaurus, 134.2 light-years from the Sun.

Other namesHIP 61622
ConstellationCentaurus
Distance134.2 light-years (41.2 pc)
Apparent magnitudemagnitude 3.85
Absolute magnitudemagnitude 0.78
Spectral typeA2V
Surface temperature9,550 K
Luminosity53.8 L☉
Radius2.68 R☉
Mass2.84 M☉ (estimated)
Right ascension (J2000)12h 37m 42.2s
Declination (J2000)−48° 32′ 29″
Space velocity (relative to the Sun)36.7 km/s

In the sky

Visible to the naked eye under a dark sky (apparent magnitude 3.85). Visible from the whole Southern Hemisphere and north to latitude 41° N. South of latitude 41° S it never sets. It stands highest at midnight in March, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1892. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 2.4 million years.

The Sun seen from there

From a planet around τ Cen, the Sun would look like a star of magnitude 7.90, in the direction where our sky has the constellation Cassiopeia. It would be invisible to the naked eye.

Neighbours

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

  • γ Cen 4.45 light-years
  • HIP 60662 5.24 light-years
  • HIP 61406 5.99 light-years
  • HIP 59926 9.01 light-years
  • HIP 61097 14.0 light-years
  • HIP 59433 14.9 light-years
  • HIP 59315 15.2 light-years
  • HIP 62749 16.0 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.