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Star · M4

GJ 3760

GJ 3760 is a main-sequence star of spectral type M4 in the constellation Canes Venatici, 80.5 light-years from the Sun.

Other namesHIP 63882
ConstellationCanes Venatici
Distance80.5 light-years (24.7 pc)
Apparent magnitudemagnitude 11.74
Absolute magnitudemagnitude 9.78
Spectral typeM4
Surface temperature3,600 K
Luminosity0.0513 L☉
Radius0.583 R☉
Mass0.476 M☉ (estimated)
Right ascension (J2000)13h 05m 29.9s
Declination (J2000)+37° 08′ 11″
Space velocity (relative to the Sun)46.4 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 11.74. Visible from the whole Northern Hemisphere and south to latitude 53° S. North of latitude 53° N it never sets. It stands highest at midnight in April, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1945. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 1.4 million years.

The Sun seen from there

From a planet around GJ 3760, the Sun would look like a star of magnitude 6.79, in the direction where our sky has the constellation Sculptor. 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.