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Star · M4

Gl 490B

Gl 490B is a main-sequence star of spectral type M4 in the constellation Canes Venatici, 65.8 light-years from the Sun.

ConstellationCanes Venatici
Distance65.8 light-years (20.2 pc)
Apparent magnitudemagnitude 13.20
Absolute magnitudemagnitude 11.68
Spectral typeM4
Surface temperature3,590 K
Luminosity0.00899 L☉
Radius0.244 R☉
Mass0.244 M☉ (estimated)
Right ascension (J2000)12h 57m 39.5s
Declination (J2000)+35° 13′ 21″
Space velocity (relative to the Sun)31.2 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 13.20. Visible from the whole Northern Hemisphere and south to latitude 55° S. North of latitude 55° 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 1960. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 1.2 million years.

The Sun seen from there

From a planet around Gl 490B, the Sun would look like a star of magnitude 6.35, in the direction where our sky has the constellation Sculptor. 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.