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Star · A0V

ε Pav

ε Pav is a main-sequence star of spectral type A0V in the constellation Pavo, 104.3 light-years from the Sun.

Other namesHIP 98495
ConstellationPavo
Distance104.3 light-years (32.0 pc)
Apparent magnitudemagnitude 3.97
Absolute magnitudemagnitude 1.44
Spectral typeA0V
Surface temperature10,540 K
Luminosity33.9 L☉
Radius1.75 R☉
Mass2.49 M☉ (estimated)
Right ascension (J2000)20h 00m 35.6s
Declination (J2000)−72° 54′ 38″
Space velocity (relative to the Sun)24.9 km/s

In the sky

Visible to the naked eye under a dark sky (apparent magnitude 3.97). Visible from the whole Southern Hemisphere and north to latitude 17° N. South of latitude 17° S it never sets. It stands highest at midnight in July, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1922. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 1.9 million years.

The Sun seen from there

From a planet around ε Pav, the Sun would look like a star of magnitude 7.36, in the direction where our sky has the constellation Camelopardalis. It would be invisible to the naked eye.

Neighbours

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

  • HIP 105612 11.9 light-years
  • CWISE J195228.45-730049.4 13.1 light-years
  • HIP 105441 16.5 light-years
  • HIP 99634 16.6 light-years
  • HIP 104299 18.3 light-years
  • HIP 109245 19.0 light-years
  • HIP 94154 19.4 light-years
  • Gl 847B 19.7 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.