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Star · K1 IIIb Fe-0.5

Algieba

Algieba is a giant star of spectral type K1 IIIb Fe-0.5 in the constellation Leo, 130.1 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).

Other namesγ¹ Leo · gam1 Leo · HIP 50583
ConstellationLeo
Distance130.1 light-years (39.9 pc)
Apparent magnitudemagnitude 2.01
Absolute magnitudemagnitude −0.99
Spectral typeK1 IIIb Fe-0.5
Surface temperature4,330 K
Luminosity324 L☉
Radius31.9 R☉
Mass1.23 M☉
Age2.4 billion years
Metallicity [Fe/H]-0.51
Right ascension (J2000)10h 19m 58.4s
Declination (J2000)+19° 50′ 29″
Space velocity (relative to the Sun)74.9 km/s

In the sky

Visible to the naked eye under a dark sky (apparent magnitude 2.01). Visible from the whole Northern Hemisphere and south to latitude 70° S. North of latitude 70° N it never sets. It stands highest at midnight in February, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1896. 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 Algieba, the Sun would look like a star of magnitude 7.83, in the direction where our sky has the constellation Aquarius. It would be invisible to the naked eye.

Planets

Neighbours

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

  • HIP 50882 6.73 light-years
  • HIP 50375 9.23 light-years
  • HIP 51874 11.0 light-years
  • HIP 48785 12.7 light-years
  • HIP 48786 12.8 light-years
  • HIP 51550 13.4 light-years
  • SIMP J10390822+2440446 14.9 light-years
  • HIP 49324 15.4 light-years

Open in the simulation

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