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Star · G5IV

HIP 60729

HIP 60729 is a subgiant star of spectral type G5IV in the constellation Centaurus, 87.6 light-years from the Sun.

ConstellationCentaurus
Distance87.6 light-years (26.9 pc)
Apparent magnitudemagnitude 6.25
Absolute magnitudemagnitude 4.10
Spectral typeG5IV
Surface temperature5,690 K
Luminosity2.15 L☉
Radius1.51 R☉
Mass1.21 M☉ (estimated)
Right ascension (J2000)12h 26m 48.1s
Declination (J2000)−48° 54′ 48″
Space velocity (relative to the Sun)87.9 km/s

In the sky

Visible to the naked eye under a dark sky (apparent magnitude 6.25). Visible from the whole Southern Hemisphere and north to latitude 41° N. South of latitude 41° 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 1938. 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 60729, the Sun would look like a star of magnitude 6.98, in the direction where our sky has the constellation Cassiopeia. 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.