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Star · F7IV

HIP 107299

HIP 107299 is a subgiant star of spectral type F7IV in the constellation Indus, 144.7 light-years from the Sun.

ConstellationIndus
Distance144.7 light-years (44.4 pc)
Apparent magnitudemagnitude 6.49
Absolute magnitudemagnitude 3.26
Spectral typeF7IV
Surface temperature6,460 K
Luminosity4.28 L☉
Radius1.65 R☉
Mass1.44 M☉ (estimated)
Right ascension (J2000)21h 43m 59.1s
Declination (J2000)−57° 19′ 31″
Space velocity (relative to the Sun)45.7 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 33° N. South of latitude 33° 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 1881. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 2.6 million years.

The Sun seen from there

From a planet around HIP 107299, the Sun would look like a star of magnitude 8.06, 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 107300 0.35 light-years
  • HIP 107806 5.68 light-years
  • HIP 106130 8.20 light-years
  • HIP 109655 10.2 light-years
  • HIP 108787 10.3 light-years
  • HIP 107476 10.4 light-years
  • HIP 108598 10.4 light-years
  • HIP 108912 11.2 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.