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Star · M4V

PSO J207.7496+29.4240

PSO J207.7496+29.4240 is a main-sequence star of spectral type M4V in the constellation Canes Venatici, 119.4 light-years from the Sun.

ConstellationCanes Venatici
Distance119.4 light-years (36.6 pc)
Apparent magnitudemagnitude 24.47
Absolute magnitudemagnitude 21.65
Spectral typeM4V
Surface temperature2,980 K
Luminosity3.43 × 10⁻⁶ L☉
Radius0.00697 R☉
Mass0.075 M☉ (estimated)
Right ascension (J2000)13h 50m 60.0s
Declination (J2000)+29° 25′ 27″
Space velocity (relative to the Sun)30.1 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 24.47. Visible from the whole Northern Hemisphere and south to latitude 61° S. North of latitude 61° 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 1907. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 2.1 million years.

The Sun seen from there

From a planet around PSO J207.7496+29.4240, the Sun would look like a star of magnitude 7.65, in the direction where our sky has the constellation Fornax. 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.