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Star · G3V

Gl 132

Gl 132 is a main-sequence star of spectral type G3V in the constellation Horologium, 80.0 light-years from the Sun.

Other namesHIP 15131
ConstellationHorologium
Distance80.0 light-years (24.5 pc)
Apparent magnitudemagnitude 6.75
Absolute magnitudemagnitude 4.80
Spectral typeG3V
Surface temperature6,020 K
Luminosity1.07 L☉
Radius0.95 R☉
Mass1.02 M☉ (estimated)
Right ascension (J2000)3h 15m 06.4s
Declination (J2000)−45° 39′ 53″
Space velocity (relative to the Sun)22.9 km/s

In the sky

Too faint for the naked eye (magnitude 6.75); binoculars will find it. Visible from the whole Southern Hemisphere and north to latitude 44° N. South of latitude 44° 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 1946. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 1.4 million years.

The Sun seen from there

From a planet around Gl 132, the Sun would look like a star of magnitude 6.78, in the direction where our sky has the constellation Boötes. 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.