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Star · A2V

HIP 103752

HIP 103752 is a main-sequence star of spectral type A2V in the constellation Pavo, 267.7 light-years from the Sun.

ConstellationPavo
Distance267.7 light-years (82.1 pc)
Apparent magnitudemagnitude 6.36
Absolute magnitudemagnitude 1.79
Spectral typeA2V
Surface temperature9,020 K
Luminosity19.6 L☉
Radius1.81 R☉
Mass2.13 M☉ (estimated)
Right ascension (J2000)21h 01m 28.0s
Declination (J2000)−68° 12′ 35″
Space velocity (relative to the Sun)10.8 km/s

In the sky

Visible to the naked eye under a dark sky (apparent magnitude 6.36). Visible from the whole Southern Hemisphere and north to latitude 22° N. South of latitude 22° S it never sets. It stands highest at midnight in August, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1758. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 4.7 million years.

The Sun seen from there

From a planet around HIP 103752, the Sun would look like a star of magnitude 9.40, in the direction where our sky has the constellation Ursa Major. It would be invisible to the naked eye.

Neighbours

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

  • HIP 102776 8.80 light-years
  • HIP 105742 10.8 light-years
  • HIP 103978 13.8 light-years
  • HIP 101006 14.8 light-years
  • HIP 104065 14.9 light-years
  • HIP 102725 15.6 light-years
  • HIP 101304 17.7 light-years
  • HIP 106855 18.1 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.