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Star · M4

Gl 465

Gl 465 is a main-sequence star of spectral type M4 in the constellation Corvus, 28.9 light-years from the Sun.

Other namesHIP 60559
ConstellationCorvus
Distance28.9 light-years (8.88 pc)
Apparent magnitudemagnitude 11.28
Absolute magnitudemagnitude 11.54
Spectral typeM4
Surface temperature3,690 K
Luminosity0.00887 L☉
Radius0.231 R☉
Mass0.243 M☉ (estimated)
Right ascension (J2000)12h 24m 52.5s
Declination (J2000)−18° 14′ 31″
Space velocity (relative to the Sun)119.0 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 11.28. Visible from the whole Southern Hemisphere and north to latitude 72° N. South of latitude 72° S 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 1997. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 513 thousand years.

The Sun seen from there

From a planet around Gl 465, the Sun would look like a star of magnitude 4.57, in the direction where our sky has the constellation Pisces. 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.