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Star · M1V

2MASS J04203904+2355502

2MASS J04203904+2355502 is a main-sequence star of spectral type M1V in the constellation Taurus, 129.8 light-years from the Sun.

ConstellationTaurus
Distance129.8 light-years (39.8 pc)
Apparent magnitudemagnitude 21.36
Absolute magnitudemagnitude 18.36
Spectral typeM1V
Surface temperature3,500 K
Luminosity2.21 × 10⁻⁵ L☉
Radius0.0128 R☉
Mass0.075 M☉ (estimated)
Right ascension (J2000)4h 20m 39.1s
Declination (J2000)+23° 55′ 47″
Space velocity (relative to the Sun)32.9 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 21.36. Visible from the whole Northern Hemisphere and south to latitude 66° S. North of latitude 66° 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 1896. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 2.3 million years.

The Sun seen from there

From a planet around 2MASS J04203904+2355502, the Sun would look like a star of magnitude 7.83, in the direction where our sky has the constellation Scorpius. 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.