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Star · G5V

HIP 42075

HIP 42075 is a main-sequence star of spectral type G5V in the constellation Pyxis, 222.0 light-years from the Sun.

ConstellationPyxis
Distance222.0 light-years (68.1 pc)
Apparent magnitudemagnitude 6.41
Absolute magnitudemagnitude 2.25
Spectral typeG5V
Surface temperature5,430 K
Luminosity12.7 L☉
Radius4.03 R☉
Mass1.89 M☉ (estimated)
Right ascension (J2000)8h 34m 31.9s
Declination (J2000)−32° 35′ 55″
Space velocity (relative to the Sun)46.5 km/s

In the sky

Visible to the naked eye under a dark sky (apparent magnitude 6.41). Visible from the whole Southern Hemisphere and north to latitude 57° N. South of latitude 57° 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 1804. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 3.9 million years.

The Sun seen from there

From a planet around HIP 42075, the Sun would look like a star of magnitude 8.99, in the direction where our sky has the constellation Cygnus. It would be invisible to the naked eye.

Neighbours

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

  • HIP 42937 8.84 light-years
  • HIP 41278 11.0 light-years
  • HIP 41477 11.8 light-years
  • HIP 43929 18.3 light-years
  • ζ Pyx 18.5 light-years
  • HIP 43509 19.0 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.