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Star · G8IV

GJ 9259

GJ 9259 is a subgiant star of spectral type G8IV in the constellation Puppis, 154.0 light-years from the Sun.

Other namesHIP 40227
ConstellationPuppis
Distance154.0 light-years (47.2 pc)
Apparent magnitudemagnitude 9.39
Absolute magnitudemagnitude 6.02
Spectral typeG8IV
Surface temperature5,220 K
Luminosity0.421 L☉
Radius0.793 R☉
Mass0.805 M☉ (estimated)
Right ascension (J2000)8h 12m 56.9s
Declination (J2000)−40° 32′ 22″
Space velocity (relative to the Sun)71.7 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 9.39. Visible from the whole Southern Hemisphere and north to latitude 49° N. South of latitude 49° 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 1872. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 2.7 million years.

The Sun seen from there

From a planet around GJ 9259, the Sun would look like a star of magnitude 8.20, 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 39102 9.48 light-years
  • HIP 41984 11.2 light-years
  • HIP 38250 12.5 light-years
  • HIP 39720 12.5 light-years
  • HIP 40174 13.3 light-years
  • HIP 42215 13.4 light-years
  • HIP 42042 14.8 light-years
  • HIP 39470 17.5 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.