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Star · B9V

υ⁴ Eri

υ⁴ Eri is a main-sequence star of spectral type B9V in the constellation Eridanus, 177.3 light-years from the Sun.

Other namesHIP 20042
ConstellationEridanus
Distance177.3 light-years (54.3 pc)
Apparent magnitudemagnitude 3.55
Absolute magnitudemagnitude −0.13
Spectral typeB9V
Surface temperature11,710 K
Luminosity175 L☉
Radius3.21 R☉
Mass3.97 M☉ (estimated)
Right ascension (J2000)4h 17m 53.7s
Declination (J2000)−33° 47′ 54″
Space velocity (relative to the Sun)24.1 km/s

In the sky

Visible to the naked eye under a dark sky (apparent magnitude 3.55). Visible from the whole Southern Hemisphere and north to latitude 56° N. South of latitude 56° S it never sets. It stands highest at midnight in November, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1849. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 3.1 million years.

The Sun seen from there

From a planet around υ⁴ Eri, the Sun would look like a star of magnitude 8.51, in the direction where our sky has the constellation Corona Borealis. It would be invisible to the naked eye.

Neighbours

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

  • HIP 20623 6.07 light-years
  • HIP 20727 7.67 light-years
  • HIP 19633 7.82 light-years
  • HIP 20002 12.4 light-years
  • HIP 20444 13.9 light-years
  • HIP 20184 16.3 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.