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Star · F9V

38 LMi

38 LMi is a main-sequence star of spectral type F9V in the constellation Leo Minor, 164.7 light-years from the Sun.

Other namesHIP 52139
ConstellationLeo Minor
Distance164.7 light-years (50.5 pc)
Apparent magnitudemagnitude 5.84
Absolute magnitudemagnitude 2.32
Spectral typeF9V
Surface temperature5,990 K
Luminosity10.6 L☉
Radius3.02 R☉
Mass1.8 M☉ (estimated)
Right ascension (J2000)10h 39m 07.6s
Declination (J2000)+37° 54′ 36″
Space velocity (relative to the Sun)54.3 km/s

In the sky

Visible to the naked eye under a dark sky (apparent magnitude 5.84). Visible from the whole Northern Hemisphere and south to latitude 52° S. North of latitude 52° N it never sets. It stands highest at midnight in February, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1861. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 2.9 million years.

The Sun seen from there

From a planet around 38 LMi, the Sun would look like a star of magnitude 8.35, in the direction where our sky has the constellation Grus. It would be invisible to the naked eye.

Neighbours

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

  • HIP 51877 9.50 light-years
  • SDSS J103321.92+400549.5 10.7 light-years
  • HIP 51312 11.3 light-years
  • HIP 53641 11.7 light-years
  • HIP 53640 11.9 light-years
  • β LMi 12.9 light-years
  • 35 LMi 14.4 light-years
  • HIP 52140 14.6 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.