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Star · K7V

Gl 707

Gl 707 is a main-sequence star of spectral type K7V in the constellation Corona Australis, 43.1 light-years from the Sun.

Other namesHIP 89211
ConstellationCorona Australis
Distance43.1 light-years (13.2 pc)
Apparent magnitudemagnitude 8.38
Absolute magnitudemagnitude 7.78
Spectral typeK7V
Surface temperature4,130 K
Luminosity0.166 L☉
Radius0.798 R☉
Mass0.639 M☉ (estimated)
Right ascension (J2000)18h 12m 21.4s
Declination (J2000)−43° 26′ 41″
Space velocity (relative to the Sun)27.7 km/s

In the sky

Too faint for the naked eye (magnitude 8.38); binoculars will find it. Visible from the whole Southern Hemisphere and north to latitude 47° N. South of latitude 47° S it never sets. It stands highest at midnight in June, 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 764 thousand years.

The Sun seen from there

From a planet around Gl 707, the Sun would look like a star of magnitude 5.43, in the direction where our sky has the constellation Auriga. 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.