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Star · G0V

10 CVn

10 CVn is a main-sequence star of spectral type G0V in the constellation Canes Venatici, 57.3 light-years from the Sun.

Other namesGl 484 · HIP 62207
ConstellationCanes Venatici
Distance57.3 light-years (17.6 pc)
Apparent magnitudemagnitude 5.95
Absolute magnitudemagnitude 4.73
Spectral typeG0V
Surface temperature6,140 K
Luminosity1.13 L☉
Radius0.939 R☉
Mass1.03 M☉ (estimated)
Right ascension (J2000)12h 44m 59.4s
Declination (J2000)+39° 16′ 45″
Space velocity (relative to the Sun)86.7 km/s

In the sky

Visible to the naked eye under a dark sky (apparent magnitude 5.95). Visible from the whole Northern Hemisphere and south to latitude 51° S. North of latitude 51° N 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 1969. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 1.0 million years.

The Sun seen from there

From a planet around 10 CVn, the Sun would look like a star of magnitude 6.05, in the direction where our sky has the constellation Sculptor. It would be visible 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.