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Star · F7V

7 CVn

7 CVn is a main-sequence star of spectral type F7V in the constellation Canes Venatici, 142.9 light-years from the Sun.

Other namesHIP 60988
ConstellationCanes Venatici
Distance142.9 light-years (43.8 pc)
Apparent magnitudemagnitude 6.21
Absolute magnitudemagnitude 3.00
Spectral typeF7V
Surface temperature6,230 K
Luminosity5.49 L☉
Radius2.01 R☉
Mass1.53 M☉ (estimated)
Right ascension (J2000)12h 30m 02.8s
Declination (J2000)+51° 32′ 08″
Space velocity (relative to the Sun)63.5 km/s

In the sky

Visible to the naked eye under a dark sky (apparent magnitude 6.21). Visible from the whole Northern Hemisphere and south to latitude 38° S. North of latitude 38° 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 1883. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 2.5 million years.

The Sun seen from there

From a planet around 7 CVn, the Sun would look like a star of magnitude 8.04, in the direction where our sky has the constellation Phoenix. 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.