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Star · M0V

GJ 1067

GJ 1067 is a main-sequence star of spectral type M0V in the constellation Camelopardalis, 84.3 light-years from the Sun.

Other namesHIP 19655
ConstellationCamelopardalis
Distance84.3 light-years (25.8 pc)
Apparent magnitudemagnitude 9.73
Absolute magnitudemagnitude 7.67
Spectral typeM0V
Surface temperature4,280 K
Luminosity0.159 L☉
Radius0.727 R☉
Mass0.632 M☉ (estimated)
Right ascension (J2000)4h 12m 42.2s
Declination (J2000)+70° 12′ 05″
Space velocity (relative to the Sun)16.4 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 9.73. Visible from the whole Northern Hemisphere and south to latitude 20° S. North of latitude 20° N it never sets. It stands highest at midnight in November, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1942. 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 1067, the Sun would look like a star of magnitude 6.89, in the direction where our sky has the constellation Triangulum Australe. 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.