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Star · M3

GJ 4079

GJ 4079 is a main-sequence star of spectral type M3 in the constellation Pavo, 54.6 light-years from the Sun.

Other namesHIP 92451
ConstellationPavo
Distance54.6 light-years (16.7 pc)
Apparent magnitudemagnitude 10.74
Absolute magnitudemagnitude 9.62
Spectral typeM3
Surface temperature3,820 K
Luminosity0.0428 L☉
Radius0.471 R☉
Mass0.455 M☉ (estimated)
Right ascension (J2000)18h 50m 26.6s
Declination (J2000)−62° 03′ 04″
Space velocity (relative to the Sun)18.3 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 10.74. Visible from the whole Southern Hemisphere and north to latitude 28° N. South of latitude 28° 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 1971. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 968 thousand years.

The Sun seen from there

From a planet around GJ 4079, the Sun would look like a star of magnitude 5.95, in the direction where our sky has the constellation Camelopardalis. 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.