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Star · G5V

Gl 722

Gl 722 is a main-sequence star of spectral type G5V in the constellation Sagittarius, 42.5 light-years from the Sun.

Other namesHIP 91438
ConstellationSagittarius
Distance42.5 light-years (13.0 pc)
Apparent magnitudemagnitude 5.85
Absolute magnitudemagnitude 5.28
Spectral typeG5V
Surface temperature5,700 K
Luminosity0.732 L☉
Radius0.879 R☉
Mass0.925 M☉ (estimated)
Right ascension (J2000)18h 38m 53.4s
Declination (J2000)−21° 03′ 07″
Space velocity (relative to the Sun)38.5 km/s

In the sky

Visible to the naked eye under a dark sky (apparent magnitude 5.85). Visible from the whole Southern Hemisphere and north to latitude 69° N. South of latitude 69° 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 754 thousand years.

The Sun seen from there

From a planet around Gl 722, the Sun would look like a star of magnitude 5.40, in the direction where our sky has the constellation Gemini. 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.