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Star · F4V

HIP 15191

HIP 15191 is a main-sequence star of spectral type F4V in the constellation Perseus, 177.1 light-years from the Sun.

ConstellationPerseus
Distance177.1 light-years (54.3 pc)
Apparent magnitudemagnitude 6.30
Absolute magnitudemagnitude 2.63
Spectral typeF4V
Surface temperature7,070 K
Luminosity7.58 L☉
Radius1.84 R☉
Mass1.66 M☉ (estimated)
Right ascension (J2000)3h 15m 47.2s
Declination (J2000)+32° 51′ 24″
Space velocity (relative to the Sun)15.5 km/s

In the sky

Visible to the naked eye under a dark sky (apparent magnitude 6.30). Visible from the whole Northern Hemisphere and south to latitude 57° S. North of latitude 57° N it never sets. It stands highest at midnight in November, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1849. 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 15191, the Sun would look like a star of magnitude 8.50, in the direction where our sky has the constellation Lupus. It would be invisible to the naked eye.

Neighbours

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

  • WISEA J030845.36+325923.1 4.90 light-years
  • HIP 14805 9.22 light-years
  • HIP 15205 9.39 light-years
  • HIP 15146 10.1 light-years
  • HIP 16517 16.1 light-years
  • HIP 14232 17.1 light-years
  • HIP 16042 18.7 light-years
  • HIP 13653 19.9 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.