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Star · B9IV

β Scl

β Scl is a subgiant star of spectral type B9IV in the constellation Sculptor, 183.2 light-years from the Sun.

Other namesHIP 116231
ConstellationSculptor
Distance183.2 light-years (56.2 pc)
Apparent magnitudemagnitude 4.38
Absolute magnitudemagnitude 0.63
Spectral typeB9IV
Surface temperature11,490 K
Luminosity83.7 L☉
Radius2.31 R☉
Mass3.22 M☉ (estimated)
Right ascension (J2000)23h 32m 58.3s
Declination (J2000)−37° 49′ 06″
Space velocity (relative to the Sun)25.0 km/s

In the sky

Visible to the naked eye under a dark sky (apparent magnitude 4.38). Visible from the whole Southern Hemisphere and north to latitude 52° N. South of latitude 52° 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 1843. 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 β Scl, the Sun would look like a star of magnitude 8.58, in the direction where our sky has the constellation Ursa Major. It would be invisible to the naked eye.

Neighbours

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

  • HIP 116293 12.2 light-years
  • HIP 115519 13.4 light-years
  • HIP 117513 14.2 light-years
  • HIP 115966 15.3 light-years
  • HIP 117091 19.7 light-years

Open in the simulation

Position, brightness and colour from the HYG / AT-HYG catalogue; temperature, luminosity, radius and mass are approximate values computed from these observations.