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Star · G3V

HIP 101345

HIP 101345 is a main-sequence star of spectral type G3V in the constellation Capricornus, 80.7 light-years from the Sun.

ConstellationCapricornus
Distance80.7 light-years (24.7 pc)
Apparent magnitudemagnitude 5.66
Absolute magnitudemagnitude 3.69
Spectral typeG3V
Surface temperature5,640 K
Luminosity3.18 L☉
Radius1.87 R☉
Mass1.34 M☉ (estimated)
Right ascension (J2000)20h 32m 23.7s
Declination (J2000)−9° 51′ 12″
Space velocity (relative to the Sun)39.6 km/s

In the sky

Visible to the naked eye under a dark sky (apparent magnitude 5.66). Visible from the whole Southern Hemisphere and north to latitude 80° N. It stands highest at midnight in July, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1945. 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 HIP 101345, the Sun would look like a star of magnitude 6.80, in the direction where our sky has the constellation Cancer. 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.