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Star · G3/5V

HD 147513

HD 147513 is a main-sequence star of spectral type G3/5V in the constellation Scorpius, 42.0 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).

Other namesGl 620.1A · HIP 80337
ConstellationScorpius
Distance42.0 light-years (12.9 pc)
Apparent magnitudemagnitude 5.37
Absolute magnitudemagnitude 4.82
Spectral typeG3/5V
Surface temperature5,880 K
Luminosity0.977 L☉
Radius0.98 R☉
Mass1.11 M☉
Age0.3 billion years
Metallicity [Fe/H]0.06
Right ascension (J2000)16h 24m 01.3s
Declination (J2000)−39° 11′ 34″
Space velocity (relative to the Sun)13.6 km/s

In the sky

Visible to the naked eye under a dark sky (apparent magnitude 5.37). Visible from the whole Southern Hemisphere and north to latitude 51° N. South of latitude 51° S it never sets. It stands highest at midnight in May, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1984. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 746 thousand years.

The Sun seen from there

From a planet around HD 147513, the Sun would look like a star of magnitude 5.38, in the direction where our sky has the constellation Perseus. It would be visible to the naked eye.

Planets

Neighbours

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

Open in the simulation

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