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Star · F2V

HIP 80719

HIP 80719 is a main-sequence star of spectral type F2V in the constellation Ophiuchus, 173.0 light-years from the Sun.

ConstellationOphiuchus
Distance173.0 light-years (53.0 pc)
Apparent magnitudemagnitude 6.49
Absolute magnitudemagnitude 2.87
Spectral typeF2V
Surface temperature6,830 K
Luminosity6.06 L☉
Radius1.76 R☉
Mass1.57 M☉ (estimated)
Right ascension (J2000)16h 28m 48.9s
Declination (J2000)−8° 07′ 44″
Space velocity (relative to the Sun)22.4 km/s

In the sky

Visible to the naked eye under a dark sky (apparent magnitude 6.49). Visible from the whole Southern Hemisphere and north to latitude 82° N. It stands highest at midnight in May, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1853. 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 HIP 80719, the Sun would look like a star of magnitude 8.45, in the direction where our sky has the constellation Taurus. It would be invisible to the naked eye.

Neighbours

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

  • HIP 80831 7.46 light-years
  • HIP 80878 11.3 light-years
  • SIMP J16133450-0747057 11.8 light-years
  • HIP 79749 12.3 light-years
  • HIP 81062 13.0 light-years
  • HIP 81347 13.1 light-years
  • HIP 80295 15.8 light-years
  • HIP 79585 19.3 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.