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Star · F4V

HIP 7189

HIP 7189 is a main-sequence star of spectral type F4V in the constellation Phoenix, 264.7 light-years from the Sun.

ConstellationPhoenix
Distance264.7 light-years (81.1 pc)
Apparent magnitudemagnitude 6.27
Absolute magnitudemagnitude 1.72
Spectral typeF4V
Surface temperature6,570 K
Luminosity17.4 L☉
Radius3.23 R☉
Mass2.06 M☉ (estimated)
Right ascension (J2000)1h 32m 36.4s
Declination (J2000)−49° 43′ 40″
Space velocity (relative to the Sun)30.7 km/s

In the sky

Visible to the naked eye under a dark sky (apparent magnitude 6.27). Visible from the whole Southern Hemisphere and north to latitude 40° N. South of latitude 40° S it never sets. It stands highest at midnight in October, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1761. 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 7189, the Sun would look like a star of magnitude 9.38, in the direction where our sky has the constellation Canes Venatici. It would be invisible to the naked eye.

Neighbours

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

  • HIP 7086 1.46 light-years
  • HIP 7136 12.0 light-years
  • HIP 7395 13.4 light-years
  • HIP 6322 13.6 light-years
  • HIP 5796 13.8 light-years
  • HIP 6949 14.6 light-years
  • HIP 8449 15.0 light-years
  • HIP 7537 15.4 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.