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Star · B9V

β¹ Tuc

β¹ Tuc is a main-sequence star of spectral type B9V in the constellation Tucana, 142.8 light-years from the Sun.

Other namesHIP 2484
ConstellationTucana
Distance142.8 light-years (43.8 pc)
Apparent magnitudemagnitude 4.36
Absolute magnitudemagnitude 1.15
Spectral typeB9V
Surface temperature11,000 K
Luminosity47.8 L☉
Radius1.9 R☉
Mass2.74 M☉ (estimated)
Right ascension (J2000)0h 31m 32.7s
Declination (J2000)−62° 57′ 30″
Space velocity (relative to the Sun)23.4 km/s

In the sky

Visible to the naked eye under a dark sky (apparent magnitude 4.36). Visible from the whole Southern Hemisphere and north to latitude 27° N. South of latitude 27° 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 1883. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 2.5 million years.

The Sun seen from there

From a planet around β¹ Tuc, the Sun would look like a star of magnitude 8.04, 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):

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.