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Star · M4V

2MASS J04183483+2131275

2MASS J04183483+2131275 is a main-sequence star of spectral type M4V in the constellation Taurus, 127.2 light-years from the Sun.

ConstellationTaurus
Distance127.2 light-years (39.0 pc)
Apparent magnitudemagnitude 22.65
Absolute magnitudemagnitude 19.69
Spectral typeM4V
Surface temperature2,980 K
Luminosity2.08 × 10⁻⁵ L☉
Radius0.0172 R☉
Mass0.075 M☉ (estimated)
Right ascension (J2000)4h 18m 34.8s
Declination (J2000)+21° 31′ 27″
Space velocity (relative to the Sun)46.9 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 22.65. Visible from the whole Northern Hemisphere and south to latitude 68° S. North of latitude 68° 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 1899. 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 J04183483+2131275, the Sun would look like a star of magnitude 7.79, 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.