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Star · G2V

Rigil Kentaurus

Rigil Kentaurus is a main-sequence star of spectral type G2V in the constellation Centaurus, 4.32 light-years from the Sun.

Other namesα¹ Cen · Gl 559A · HIP 71683
ConstellationCentaurus
Distance4.32 light-years (1.32 pc)
Apparent magnitudemagnitude −0.01
Absolute magnitudemagnitude 4.38
Spectral typeG2V
Surface temperature5,570 K
Luminosity1.72 L☉
Radius1.41 R☉
Mass1.15 M☉ (estimated)
Right ascension (J2000)14h 39m 36.5s
Declination (J2000)−60° 50′ 02″
Space velocity (relative to the Sun)28.1 km/s

In the sky

Visible to the naked eye under a dark sky (apparent magnitude −0.01). Visible from the whole Southern Hemisphere and north to latitude 29° N. South of latitude 29° S it never sets. It stands highest at midnight in April, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 2022. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 77 thousand years.

The Sun seen from there

From a planet around Rigil Kentaurus, the Sun would look like a star of magnitude 0.44, in the direction where our sky has the constellation Cassiopeia. 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.