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Star · F9V

Gl 540.3

Gl 540.3 is a main-sequence star of spectral type F9V in the constellation Centaurus, 68.2 light-years from the Sun.

Other namesHIP 69671
ConstellationCentaurus
Distance68.2 light-years (20.9 pc)
Apparent magnitudemagnitude 6.31
Absolute magnitudemagnitude 4.71
Spectral typeF9V
Surface temperature5,980 K
Luminosity1.17 L☉
Radius1.01 R☉
Mass1.04 M☉ (estimated)
Right ascension (J2000)14h 15m 38.7s
Declination (J2000)−45° 00′ 03″
Space velocity (relative to the Sun)19.2 km/s

In the sky

Visible to the naked eye under a dark sky (apparent magnitude 6.31). Visible from the whole Southern Hemisphere and north to latitude 45° N. South of latitude 45° 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 1958. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 1.2 million years.

The Sun seen from there

From a planet around Gl 540.3, the Sun would look like a star of magnitude 6.43, in the direction where our sky has the constellation Andromeda. 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.