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Star · M4V

SDSS J140347.84+351313.1

SDSS J140347.84+351313.1 is a main-sequence star of spectral type M4V in the constellation Canes Venatici, 293.5 light-years from the Sun.

ConstellationCanes Venatici
Distance293.5 light-years (90.0 pc)
Apparent magnitudemagnitude 21.91
Absolute magnitudemagnitude 17.14
Spectral typeM4V
Surface temperature2,980 K
Luminosity2.19 × 10⁻⁴ L☉
Radius0.0557 R☉
Mass0.075 M☉ (estimated)
Right ascension (J2000)14h 03m 47.9s
Declination (J2000)+35° 13′ 13″
Space velocity (relative to the Sun)122.8 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 21.91. 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 1732. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 5.2 million years.

The Sun seen from there

From a planet around SDSS J140347.84+351313.1, the Sun would look like a star of magnitude 9.60, 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.