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Star · G5 III/IV

HD 1397

HD 1397 is a main-sequence star of spectral type G5 III/IV in the constellation Tucana, 261.1 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).

Other namesHIP 1419
ConstellationTucana
Distance261.1 light-years (80.0 pc)
Apparent magnitudemagnitude 7.79
Absolute magnitudemagnitude 3.27
Spectral typeG5 III/IV
Surface temperature5,520 K
Luminosity4.57 L☉
Radius2.34 R☉
Mass1.32 M☉
Age4.5 billion years
Metallicity [Fe/H]0.29
Right ascension (J2000)0h 17m 47.1s
Declination (J2000)−66° 21′ 32″
Space velocity (relative to the Sun)39.3 km/s

In the sky

Too faint for the naked eye (magnitude 7.79); binoculars will find it. Visible from the whole Southern Hemisphere and north to latitude 24° N. South of latitude 24° S it never sets. It stands highest at midnight in September, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1765. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 4.6 million years.

The Sun seen from there

From a planet around HD 1397, the Sun would look like a star of magnitude 9.35, 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 1572 12.6 light-years
  • HIP 1258 13.1 light-years
  • HIP 494 16.4 light-years
  • HIP 2111 16.8 light-years
  • HIP 1394 17.4 light-years
  • HIP 118179 18.0 light-years
  • HIP 1672 19.9 light-years

Open in the simulation

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