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Star · F3V

HIP 24017

HIP 24017 is a main-sequence star of spectral type F3V in the constellation Camelopardalis, 127.5 light-years from the Sun.

ConstellationCamelopardalis
Distance127.5 light-years (39.1 pc)
Apparent magnitudemagnitude 6.37
Absolute magnitudemagnitude 3.41
Spectral typeF3V
Surface temperature6,630 K
Luminosity3.68 L☉
Radius1.45 R☉
Mass1.39 M☉ (estimated)
Right ascension (J2000)5h 09m 44.6s
Declination (J2000)+64° 55′ 10″
Space velocity (relative to the Sun)34.0 km/s

In the sky

Visible to the naked eye under a dark sky (apparent magnitude 6.37). Visible from the whole Northern Hemisphere and south to latitude 25° S. North of latitude 25° N it never sets. It stands highest at midnight in December, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1899. 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 24017, the Sun would look like a star of magnitude 7.79, in the direction where our sky has the constellation Ara. It would be invisible to the naked eye.

Neighbours

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

  • HIP 25354 5.25 light-years
  • HIP 22961 5.52 light-years
  • HIP 22615 5.55 light-years
  • HIP 21921 7.33 light-years
  • HIP 25222 8.20 light-years
  • HIP 25233 11.9 light-years
  • HIP 21750 13.5 light-years
  • HIP 19959 13.7 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.