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Star · G9 III

υ Leo

υ Leo is a giant star of spectral type G9 III in the constellation Leo, 177.8 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).

Other namesups Leo · HIP 56647
ConstellationLeo
Distance177.8 light-years (54.5 pc)
Apparent magnitudemagnitude 4.30
Absolute magnitudemagnitude 0.62
Spectral typeG9 III
Surface temperature4,840 K
Luminosity63.1 L☉
Radius11.2 R☉
Mass1.48 M☉
Metallicity [Fe/H]-0.20
Right ascension (J2000)11h 36m 56.9s
Declination (J2000)−0° 49′ 25″
Space velocity (relative to the Sun)11.3 km/s

In the sky

Visible to the naked eye under a dark sky (apparent magnitude 4.30). Visible from the whole Southern Hemisphere and north to latitude 89° N. 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 1848. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 3.2 million years.

The Sun seen from there

From a planet around υ Leo, the Sun would look like a star of magnitude 8.51, in the direction where our sky has the constellation Pisces. It would be invisible 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.