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Star · G0V

ι Per

ι Per is a main-sequence star of spectral type G0V in the constellation Perseus, 34.5 light-years from the Sun.

Other namesGl 124 · HIP 14632
ConstellationPerseus
Distance34.5 light-years (10.6 pc)
Apparent magnitudemagnitude 4.05
Absolute magnitudemagnitude 3.93
Spectral typeG0V
Surface temperature5,990 K
Luminosity2.41 L☉
Radius1.44 R☉
Mass1.25 M☉ (estimated)
Right ascension (J2000)3h 09m 04.1s
Declination (J2000)+49° 36′ 48″
Space velocity (relative to the Sun)80.4 km/s

In the sky

Visible to the naked eye under a dark sky (apparent magnitude 4.05). Visible from the whole Northern Hemisphere and south to latitude 40° S. North of latitude 40° 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 1992. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 612 thousand years.

The Sun seen from there

From a planet around ι Per, the Sun would look like a star of magnitude 4.95, in the direction where our sky has the constellation Lupus. It would be visible to the naked eye.

Neighbours

Its nearest neighbours in the catalogue (within 20 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.