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Star · A5V

24 CVn

24 CVn is a main-sequence star of spectral type A5V in the constellation Canes Venatici, 185.4 light-years from the Sun.

Other namesHIP 66234
ConstellationCanes Venatici
Distance185.4 light-years (56.8 pc)
Apparent magnitudemagnitude 4.68
Absolute magnitudemagnitude 0.91
Spectral typeA5V
Surface temperature8,730 K
Luminosity42.5 L☉
Radius2.85 R☉
Mass2.65 M☉ (estimated)
Right ascension (J2000)13h 34m 27.3s
Declination (J2000)+49° 00′ 58″
Space velocity (relative to the Sun)39.6 km/s

In the sky

Visible to the naked eye under a dark sky (apparent magnitude 4.68). Visible from the whole Northern Hemisphere and south to latitude 41° S. North of latitude 41° 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 1841. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 3.3 million years.

The Sun seen from there

From a planet around 24 CVn, the Sun would look like a star of magnitude 8.60, 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):

  • HIP 65276 8.76 light-years
  • HIP 68066 12.0 light-years
  • HIP 65641 14.9 light-years
  • HIP 65407 16.1 light-years
  • SDSS J130234.71+512600.9 18.2 light-years
  • HIP 66804 18.9 light-years
  • HIP 68193 19.4 light-years
  • HIP 67590 19.6 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.