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Star · B8V

ν Dor

ν Dor is a main-sequence star of spectral type B8V in the constellation Dorado, 281.8 light-years from the Sun.

Other namesHIP 29134
ConstellationDorado
Distance281.8 light-years (86.4 pc)
Apparent magnitudemagnitude 5.06
Absolute magnitudemagnitude 0.38
Spectral typeB8V
Surface temperature11,120 K
Luminosity99.7 L☉
Radius2.69 R☉
Mass3.38 M☉ (estimated)
Right ascension (J2000)6h 08m 44.3s
Declination (J2000)−68° 50′ 36″
Space velocity (relative to the Sun)28.7 km/s

In the sky

Visible to the naked eye under a dark sky (apparent magnitude 5.06). Visible from the whole Southern Hemisphere and north to latitude 21° N. South of latitude 21° S it never sets. It stands highest at midnight in December, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1744. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 5.0 million years.

The Sun seen from there

From a planet around ν Dor, the Sun would look like a star of magnitude 9.51, in the direction where our sky has the constellation Draco. It would be invisible to the naked eye.

Neighbours

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

  • π² Dor 9.41 light-years
  • HIP 30516 9.47 light-years
  • HIP 30050 16.0 light-years
  • HIP 31021 17.1 light-years
  • HIP 26904 18.8 light-years
  • HIP 25811 19.3 light-years
  • HIP 25805 19.4 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.