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Star · K0 V

HD 39194

HD 39194 is a main-sequence star of spectral type K0 V in the constellation Mensa, 86.2 light-years from the Sun. It is orbited by 3 confirmed exoplanet(s).

Other namesGl 217.2 · HIP 27080
ConstellationMensa
Distance86.2 light-years (26.4 pc)
Apparent magnitudemagnitude 8.09
Absolute magnitudemagnitude 5.98
Spectral typeK0 V
Surface temperature5,210 K
Luminosity0.39 L☉
Radius0.784 R☉
Mass0.86 M☉
Age10.0 billion years
Metallicity [Fe/H]-0.61
Right ascension (J2000)5h 44m 32.3s
Declination (J2000)−70° 08′ 37″
Space velocity (relative to the Sun)160.7 km/s

In the sky

Too faint for the naked eye (magnitude 8.09); binoculars will find it. Visible from the whole Southern Hemisphere and north to latitude 20° N. South of latitude 20° S 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 1940. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 1.5 million years.

The Sun seen from there

From a planet around HD 39194, the Sun would look like a star of magnitude 6.94, in the direction where our sky has the constellation Draco. It would be invisible to the naked eye.

Planets

Neighbours

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

  • HIP 31134 8.63 light-years
  • GJ 9206 9.32 light-years
  • GJ 3397 11.1 light-years
  • Gl 224.1 11.3 light-years
  • HIP 34712 13.5 light-years
  • HIP 28964 13.5 light-years
  • GJ 3344 14.2 light-years
  • GJ 9202 16.6 light-years

Open in the simulation

Stellar parameters from the NASA Exoplanet Archive; position and brightness from the HYG / AT-HYG catalogue.