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Star · K4

Gl 868

Gl 868 is a main-sequence star of spectral type K4 in the constellation Piscis Austrinus, 43.3 light-years from the Sun.

Other namesHIP 111960
ConstellationPiscis Austrinus
Distance43.3 light-years (13.3 pc)
Apparent magnitudemagnitude 7.83
Absolute magnitudemagnitude 7.21
Spectral typeK4
Surface temperature4,420 K
Luminosity0.215 L☉
Radius0.79 R☉
Mass0.681 M☉ (estimated)
Right ascension (J2000)22h 40m 43.4s
Declination (J2000)−29° 40′ 28″
Space velocity (relative to the Sun)24.0 km/s

In the sky

Too faint for the naked eye (magnitude 7.83); binoculars will find it. Visible from the whole Southern Hemisphere and north to latitude 60° N. South of latitude 60° 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 1983. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 768 thousand years.

The Sun seen from there

From a planet around Gl 868, the Sun would look like a star of magnitude 5.45, 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.