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Star · K1V

GJ 4087

GJ 4087 is a main-sequence star of spectral type K1V in the constellation Corona Australis, 85.7 light-years from the Sun.

Other namesHIP 92858
ConstellationCorona Australis
Distance85.7 light-years (26.3 pc)
Apparent magnitudemagnitude 7.98
Absolute magnitudemagnitude 5.88
Spectral typeK1V
Surface temperature5,110 K
Luminosity0.497 L☉
Radius0.898 R☉
Mass0.84 M☉ (estimated)
Right ascension (J2000)18h 55m 18.8s
Declination (J2000)−37° 29′ 54″
Space velocity (relative to the Sun)53.0 km/s

In the sky

Too faint for the naked eye (magnitude 7.98); binoculars will find it. Visible from the whole Southern Hemisphere and north to latitude 53° N. South of latitude 53° S it never sets. It stands highest at midnight in July, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1940. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 1.5 million years.

The Sun seen from there

From a planet around GJ 4087, the Sun would look like a star of magnitude 6.93, in the direction where our sky has the constellation Auriga. 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.