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Star · A9III

17 CVn

17 CVn is a giant star of spectral type A9III in the constellation Canes Venatici, 195.0 light-years from the Sun.

Other namesHIP 64246
ConstellationCanes Venatici
Distance195.0 light-years (59.8 pc)
Apparent magnitudemagnitude 5.91
Absolute magnitudemagnitude 2.03
Spectral typeA9III
Surface temperature7,500 K
Luminosity13.4 L☉
Radius2.17 R☉
Mass1.91 M☉ (estimated)
Right ascension (J2000)13h 10m 03.2s
Declination (J2000)+38° 29′ 56″
Space velocity (relative to the Sun)28.7 km/s

In the sky

Visible to the naked eye under a dark sky (apparent magnitude 5.91). Visible from the whole Northern Hemisphere and south to latitude 52° S. North of latitude 52° N 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 1831. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 3.5 million years.

The Sun seen from there

From a planet around 17 CVn, the Sun would look like a star of magnitude 8.71, in the direction where our sky has the constellation Sculptor. It would be invisible to the naked eye.

Neighbours

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

  • HIP 64484 4.35 light-years
  • HIP 64928 8.37 light-years
  • HIP 65114 9.54 light-years
  • HIP 64469 13.3 light-years
  • HIP 64028 14.0 light-years
  • HIP 64461 16.0 light-years
  • HIP 64979 17.0 light-years
  • 2MASS J13264464+3627407 17.2 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.