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Star · G8IV

HIP 106907

HIP 106907 is a subgiant star of spectral type G8IV in the constellation Piscis Austrinus, 143.8 light-years from the Sun.

ConstellationPiscis Austrinus
Distance143.8 light-years (44.1 pc)
Apparent magnitudemagnitude 6.28
Absolute magnitudemagnitude 3.06
Spectral typeG8IV
Surface temperature4,870 K
Luminosity7.48 L☉
Radius3.85 R☉
Mass1.65 M☉ (estimated)
Right ascension (J2000)21h 39m 06.1s
Declination (J2000)−33° 40′ 44″
Space velocity (relative to the Sun)25.8 km/s

In the sky

Visible to the naked eye under a dark sky (apparent magnitude 6.28). Visible from the whole Southern Hemisphere and north to latitude 56° N. South of latitude 56° 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 1882. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 2.6 million years.

The Sun seen from there

From a planet around HIP 106907, the Sun would look like a star of magnitude 8.05, in the direction where our sky has the constellation Leo Minor. 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.