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Star · M3V

2MASS J04134574+3709087

2MASS J04134574+3709087 is a main-sequence star of spectral type M3V in the constellation Perseus, 62.8 light-years from the Sun.

ConstellationPerseus
Distance62.8 light-years (19.3 pc)
Apparent magnitudemagnitude 21.20
Absolute magnitudemagnitude 19.78
Spectral typeM3V
Surface temperature3,140 K
Luminosity1.26 × 10⁻⁵ L☉
Radius0.012 R☉
Mass0.075 M☉ (estimated)
Right ascension (J2000)4h 13m 46.6s
Declination (J2000)+37° 09′ 05″
Space velocity (relative to the Sun)62.6 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 21.20. Visible from the whole Northern Hemisphere and south to latitude 53° S. North of latitude 53° N it never sets. It stands highest at midnight in November, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1963. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 1.1 million years.

The Sun seen from there

From a planet around 2MASS J04134574+3709087, the Sun would look like a star of magnitude 6.25, in the direction where our sky has the constellation Scorpius. 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.