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Star · F6V

τ PsA

τ PsA is a main-sequence star of spectral type F6V in the constellation Piscis Austrinus, 60.2 light-years from the Sun.

Other namesGl 849.1 · HIP 109422
ConstellationPiscis Austrinus
Distance60.2 light-years (18.5 pc)
Apparent magnitudemagnitude 4.94
Absolute magnitudemagnitude 3.61
Spectral typeF6V
Surface temperature6,440 K
Luminosity3.09 L☉
Radius1.41 R☉
Mass1.33 M☉ (estimated)
Right ascension (J2000)22h 10m 08.8s
Declination (J2000)−32° 32′ 54″
Space velocity (relative to the Sun)40.9 km/s

In the sky

Visible to the naked eye under a dark sky (apparent magnitude 4.94). Visible from the whole Southern Hemisphere and north to latitude 57° N. South of latitude 57° S it never sets. It stands highest at midnight in August, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1966. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 1.1 million years.

The Sun seen from there

From a planet around τ PsA, the Sun would look like a star of magnitude 6.16, in the direction where our sky has the constellation Leo Minor. It would be visible 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.