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Star · G2

HD 105779

HD 105779 is a main-sequence star of spectral type G2 in the constellation Corvus, 179.7 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).

Other namesHIP 59357
ConstellationCorvus
Distance179.7 light-years (55.1 pc)
Apparent magnitudemagnitude 8.65
Absolute magnitudemagnitude 4.94
Spectral typeG2
Surface temperature5,790 K
Luminosity0.78 L☉
Radius0.94 R☉
Mass0.89 M☉
Age7.5 billion years
Metallicity [Fe/H]-0.25
Right ascension (J2000)12h 10m 39.0s
Declination (J2000)−16° 57′ 23″
Space velocity (relative to the Sun)67.0 km/s

In the sky

Too faint for the naked eye (magnitude 8.65); binoculars will find it. Visible from the whole Southern Hemisphere and north to latitude 73° N. South of latitude 73° S it never sets. It stands highest at midnight in March, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1846. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 3.2 million years.

The Sun seen from there

From a planet around HD 105779, the Sun would look like a star of magnitude 8.54, in the direction where our sky has the constellation Pegasus. It would be invisible to the naked eye.

Planets

Neighbours

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

  • TOI-782 11.7 light-years
  • SIMP J12184982-1332525 14.0 light-years
  • HIP 58515 14.8 light-years
  • HIP 58152 15.2 light-years
  • HIP 58894 17.6 light-years
  • HIP 60802 18.7 light-years
  • HD 103774 18.9 light-years
  • HIP 60620 19.8 light-years

Open in the simulation

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