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Star · K9 V

HD 113538

HD 113538 is a main-sequence star of spectral type K9 V in the constellation Centaurus, 53.2 light-years from the Sun. It is orbited by 2 confirmed exoplanet(s).

Other namesGl 496.1 · HIP 63833
ConstellationCentaurus
Distance53.2 light-years (16.3 pc)
Apparent magnitudemagnitude 9.05
Absolute magnitudemagnitude 7.99
Spectral typeK9 V
Surface temperature4,460 K
Luminosity0.09 L☉
Radius0.53 R☉
Mass0.585 M☉
Age4.3 billion years
Metallicity [Fe/H]-0.24
Right ascension (J2000)13h 04m 57.8s
Declination (J2000)−52° 26′ 35″
Space velocity (relative to the Sun)94.8 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 9.05. Visible from the whole Southern Hemisphere and north to latitude 38° N. South of latitude 38° 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 1973. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 944 thousand years.

The Sun seen from there

From a planet around HD 113538, the Sun would look like a star of magnitude 5.89, in the direction where our sky has the constellation Cassiopeia. It would be visible to the naked eye.

Planets

Neighbours

Its nearest neighbours in the catalogue (within 20 light-years):

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Stellar parameters from the NASA Exoplanet Archive; position and brightness from the HYG / AT-HYG catalogue.