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Star · F3IV

HIP 22850

HIP 22850 is a subgiant star of spectral type F3IV in the constellation Taurus, 204.1 light-years from the Sun.

ConstellationTaurus
Distance204.1 light-years (62.6 pc)
Apparent magnitudemagnitude 6.36
Absolute magnitudemagnitude 2.38
Spectral typeF3IV
Surface temperature7,510 K
Luminosity9.72 L☉
Radius1.84 R☉
Mass1.77 M☉ (estimated)
Right ascension (J2000)4h 54m 58.4s
Declination (J2000)+19° 29′ 07″
Space velocity (relative to the Sun)46.3 km/s

In the sky

Visible to the naked eye under a dark sky (apparent magnitude 6.36). Visible from the whole Northern Hemisphere and south to latitude 71° S. North of latitude 71° N it never sets. It stands highest at midnight in December, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1822. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 3.6 million years.

The Sun seen from there

From a planet around HIP 22850, the Sun would look like a star of magnitude 8.81, in the direction where our sky has the constellation Ophiuchus. It would be invisible to the naked eye.

Neighbours

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

  • 106 Tau 11.3 light-years
  • HIP 22566 15.2 light-years
  • HIP 22972 15.7 light-years
  • HIP 22782 16.7 light-years
  • HIP 21403 16.7 light-years
  • HIP 21503 17.9 light-years
  • HIP 21788 19.4 light-years
  • HIP 21741 19.5 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.