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Star · K3 V

HD 215497

HD 215497 is a main-sequence star of spectral type K3 V in the constellation Tucana, 132.3 light-years from the Sun. It is orbited by 2 confirmed exoplanet(s).

Other namesHIP 112441
ConstellationTucana
Distance132.3 light-years (40.6 pc)
Apparent magnitudemagnitude 8.96
Absolute magnitudemagnitude 5.92
Spectral typeK3 V
Surface temperature5,110 K
Luminosity0.389 L☉
Radius0.85 R☉
Mass0.92 M☉
Age5.8 billion years
Metallicity [Fe/H]0.23
Right ascension (J2000)22h 46m 36.7s
Declination (J2000)−56° 35′ 58″
Space velocity (relative to the Sun)51.6 km/s

In the sky

Too faint for the naked eye (magnitude 8.96); binoculars will find it. Visible from the whole Southern Hemisphere and north to latitude 33° N. South of latitude 33° S it never sets. It stands highest at midnight in August, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1894. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 2.3 million years.

The Sun seen from there

From a planet around HD 215497, the Sun would look like a star of magnitude 7.87, in the direction where our sky has the constellation Ursa Major. It would be invisible to the naked eye.

Planets

Neighbours

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

  • GJ 9819 11.2 light-years
  • HIP 112703 12.5 light-years
  • HIP 114736 12.9 light-years
  • ε Gru 13.3 light-years
  • HIP 113596 15.1 light-years
  • HIP 114167 15.6 light-years
  • HIP 109655 15.7 light-years
  • HD 213240 17.5 light-years

Open in the simulation

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