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Star · F5IV

κ Ret

κ Ret is a subgiant star of spectral type F5IV in the constellation Reticulum, 71.0 light-years from the Sun.

Other namesGl 143.2A · HIP 16245
ConstellationReticulum
Distance71.0 light-years (21.8 pc)
Apparent magnitudemagnitude 4.71
Absolute magnitudemagnitude 3.02
Spectral typeF5IV
Surface temperature6,830 K
Luminosity5.26 L☉
Radius1.64 R☉
Mass1.51 M☉ (estimated)
Right ascension (J2000)3h 29m 22.7s
Declination (J2000)−62° 56′ 15″
Space velocity (relative to the Sun)56.8 km/s

In the sky

Visible to the naked eye under a dark sky (apparent magnitude 4.71). Visible from the whole Southern Hemisphere and north to latitude 27° N. South of latitude 27° S 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 1955. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 1.3 million years.

The Sun seen from there

From a planet around κ Ret, the Sun would look like a star of magnitude 6.52, in the direction where our sky has the constellation Draco. It would be invisible 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.