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Star · M0V

Gl 462

Gl 462 is a main-sequence star of spectral type M0V in the constellation Canes Venatici, 52.0 light-years from the Sun.

Other namesHIP 60303
ConstellationCanes Venatici
Distance52.0 light-years (15.9 pc)
Apparent magnitudemagnitude 9.36
Absolute magnitudemagnitude 8.35
Spectral typeM0V
Surface temperature4,030 K
Luminosity0.109 L☉
Radius0.678 R☉
Mass0.574 M☉ (estimated)
Right ascension (J2000)12h 21m 54.0s
Declination (J2000)+42° 08′ 02″
Space velocity (relative to the Sun)43.2 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 9.36. Visible from the whole Northern Hemisphere and south to latitude 48° S. North of latitude 48° N it never sets. It stands highest at midnight in March, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1974. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 922 thousand years.

The Sun seen from there

From a planet around Gl 462, the Sun would look like a star of magnitude 5.84, in the direction where our sky has the constellation Phoenix. 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.