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Star · G4IV

HIP 61379

HIP 61379 is a subgiant star of spectral type G4IV in the constellation Centaurus, 92.8 light-years from the Sun.

ConstellationCentaurus
Distance92.8 light-years (28.5 pc)
Apparent magnitudemagnitude 5.76
Absolute magnitudemagnitude 3.49
Spectral typeG4IV
Surface temperature5,660 K
Luminosity3.82 L☉
Radius2.03 R☉
Mass1.4 M☉ (estimated)
Right ascension (J2000)12h 34m 42.4s
Declination (J2000)−44° 40′ 23″
Space velocity (relative to the Sun)34.8 km/s

In the sky

Visible to the naked eye under a dark sky (apparent magnitude 5.76). 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 March, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1933. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 1.6 million years.

The Sun seen from there

From a planet around HIP 61379, the Sun would look like a star of magnitude 7.10, in the direction where our sky has the constellation Andromeda. 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.