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Star · M5V

Gl 268

Gl 268 is a main-sequence star of spectral type M5V in the constellation Auriga, 19.7 light-years from the Sun.

Other namesHIP 34603
ConstellationAuriga
Distance19.7 light-years (6.05 pc)
Apparent magnitudemagnitude 11.65
Absolute magnitudemagnitude 12.74
Spectral typeM5V
Surface temperature3,520 K
Luminosity0.00384 L☉
Radius0.167 R☉
Mass0.169 M☉ (estimated)
Right ascension (J2000)7h 10m 01.8s
Declination (J2000)+38° 31′ 46″
Space velocity (relative to the Sun)48.2 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 11.65. Visible from the whole Northern Hemisphere and south to latitude 51° S. North of latitude 51° N it never sets. It stands highest at midnight in January, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 2006. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 350 thousand years.

The Sun seen from there

From a planet around Gl 268, the Sun would look like a star of magnitude 3.74, in the direction where our sky has the constellation Corona Australis. 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.