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Star · A

HIP 105913

HIP 105913 is a main-sequence star of spectral type A in the constellation Microscopium, 176.4 light-years from the Sun.

ConstellationMicroscopium
Distance176.4 light-years (54.1 pc)
Apparent magnitudemagnitude 5.50
Absolute magnitudemagnitude 1.83
Spectral typeA
Surface temperature6,920 K
Luminosity15.7 L☉
Radius2.75 R☉
Mass1.99 M☉ (estimated)
Right ascension (J2000)21h 27m 01.6s
Declination (J2000)−42° 32′ 52″
Space velocity (relative to the Sun)28.7 km/s

In the sky

Visible to the naked eye under a dark sky (apparent magnitude 5.50). Visible from the whole Southern Hemisphere and north to latitude 47° N. South of latitude 47° 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 1850. 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 105913, the Sun would look like a star of magnitude 8.50, 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 105327 5.11 light-years
  • HIP 105863 7.29 light-years
  • HIP 107362 10.5 light-years
  • HIP 105391 12.4 light-years
  • HIP 106782 14.4 light-years
  • HIP 103710 15.3 light-years
  • θ¹ Mic 15.9 light-years
  • HIP 107779 18.2 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.