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Star · F3V

HIP 33478

HIP 33478 is a main-sequence star of spectral type F3V in the constellation Canis Major, 132.0 light-years from the Sun.

ConstellationCanis Major
Distance132.0 light-years (40.5 pc)
Apparent magnitudemagnitude 5.45
Absolute magnitudemagnitude 2.41
Spectral typeF3V
Surface temperature6,930 K
Luminosity9.19 L☉
Radius2.1 R☉
Mass1.74 M☉ (estimated)
Right ascension (J2000)6h 57m 33.9s
Declination (J2000)−24° 37′ 51″
Space velocity (relative to the Sun)28.3 km/s

In the sky

Visible to the naked eye under a dark sky (apparent magnitude 5.45). Visible from the whole Southern Hemisphere and north to latitude 65° N. South of latitude 65° S it never sets. It stands highest at midnight in January, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1894. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 2.3 million years.

The Sun seen from there

From a planet around HIP 33478, the Sun would look like a star of magnitude 7.87, in the direction where our sky has the constellation Vulpecula. It would be invisible to the naked eye.

Neighbours

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

  • HIP 33020 8.00 light-years
  • HIP 34879 15.3 light-years
  • HD 47186 16.1 light-years
  • HIP 33691 16.6 light-years
  • HIP 33705 16.6 light-years
  • HIP 36347 18.1 light-years
  • HIP 33654 18.7 light-years
  • HIP 33799 19.5 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.