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Star · G8/K0

Lusitânia

Lusitânia is a main-sequence star of spectral type G8/K0 in the constellation Monoceros, 113.9 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).

Other namesHD 45652 · HIP 30905
ConstellationMonoceros
Distance113.9 light-years (34.9 pc)
Apparent magnitudemagnitude 8.10
Absolute magnitudemagnitude 5.39
Spectral typeG8/K0
Surface temperature5,290 K
Luminosity0.631 L☉
Radius0.94 R☉
Mass0.92 M☉
Age8.4 billion years
Metallicity [Fe/H]0.26
Right ascension (J2000)6h 29m 13.2s
Declination (J2000)+10° 56′ 02″
Space velocity (relative to the Sun)36.1 km/s

In the sky

Too faint for the naked eye (magnitude 8.10); binoculars will find it. Visible from the whole Northern Hemisphere and south to latitude 79° S. North of latitude 79° N 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 1912. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 2.0 million years.

The Sun seen from there

From a planet around Lusitânia, the Sun would look like a star of magnitude 7.54, in the direction where our sky has the constellation Scutum. It would be invisible to the naked eye.

Planets

Neighbours

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

  • HIP 30552 5.79 light-years
  • HIP 29132 10.5 light-years
  • HIP 31069 10.7 light-years
  • Alhena 12.2 light-years
  • HIP 29063 12.6 light-years
  • HIP 29001 17.3 light-years
  • HIP 31655 17.7 light-years
  • UGPS J065227.71+032431.0 18.8 light-years

Open in the simulation

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