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Star · M0V

Gl 488

Gl 488 is a main-sequence star of spectral type M0V in the constellation Virgo, 34.8 light-years from the Sun.

Other namesHIP 62687
ConstellationVirgo
Distance34.8 light-years (10.7 pc)
Apparent magnitudemagnitude 8.49
Absolute magnitudemagnitude 8.35
Spectral typeM0V
Surface temperature3,940 K
Luminosity0.12 L☉
Radius0.746 R☉
Mass0.589 M☉ (estimated)
Right ascension (J2000)12h 50m 43.5s
Declination (J2000)−0° 46′ 05″
Space velocity (relative to the Sun)20.6 km/s

In the sky

Too faint for the naked eye (magnitude 8.49); binoculars will find it. Visible from the whole Southern Hemisphere and north to latitude 89° N. 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 1991. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 616 thousand years.

The Sun seen from there

From a planet around Gl 488, the Sun would look like a star of magnitude 4.97, in the direction where our sky has the constellation Cetus. 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.