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Star · F6IV

HIP 114167

HIP 114167 is a subgiant star of spectral type F6IV in the constellation Grus, 134.1 light-years from the Sun.

ConstellationGrus
Distance134.1 light-years (41.1 pc)
Apparent magnitudemagnitude 5.81
Absolute magnitudemagnitude 2.74
Spectral typeF6IV
Surface temperature6,450 K
Luminosity6.88 L☉
Radius2.1 R☉
Mass1.62 M☉ (estimated)
Right ascension (J2000)23h 07m 14.8s
Declination (J2000)−50° 41′ 12″
Space velocity (relative to the Sun)9.2 km/s

In the sky

Visible to the naked eye under a dark sky (apparent magnitude 5.81). Visible from the whole Southern Hemisphere and north to latitude 39° N. South of latitude 39° S it never sets. It stands highest at midnight in September, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1892. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 2.4 million years.

The Sun seen from there

From a planet around HIP 114167, the Sun would look like a star of magnitude 7.90, 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 114736 9.34 light-years
  • ε Gru 10.2 light-years
  • HIP 112414 10.2 light-years
  • HIP 115577 10.9 light-years
  • HIP 112908 10.9 light-years
  • HIP 112843 11.8 light-years
  • HIP 113596 12.0 light-years
  • HIP 113190 13.9 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.