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Star · A5IV

HIP 109404

HIP 109404 is a subgiant star of spectral type A5IV in the constellation Piscis Austrinus, 209.9 light-years from the Sun.

ConstellationPiscis Austrinus
Distance209.9 light-years (64.4 pc)
Apparent magnitudemagnitude 5.37
Absolute magnitudemagnitude 1.33
Spectral typeA5IV
Surface temperature7,860 K
Luminosity26.3 L☉
Radius2.76 R☉
Mass2.31 M☉ (estimated)
Right ascension (J2000)22h 09m 55.7s
Declination (J2000)−34° 00′ 54″
Space velocity (relative to the Sun)9.9 km/s

In the sky

Visible to the naked eye under a dark sky (apparent magnitude 5.37). Visible from the whole Southern Hemisphere and north to latitude 56° N. South of latitude 56° 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 1816. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 3.7 million years.

The Sun seen from there

From a planet around HIP 109404, the Sun would look like a star of magnitude 8.87, in the direction where our sky has the constellation Leo Minor. It would be invisible to the naked eye.

Neighbours

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

  • HIP 110262 11.4 light-years
  • HIP 109007 11.6 light-years
  • HIP 109462 14.9 light-years
  • HIP 109470 16.1 light-years
  • HIP 109207 16.1 light-years
  • HIP 110028 16.4 light-years
  • HIP 109149 18.9 light-years
  • ι PsA 19.7 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.