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Star · M4V

2MASS J04062677-3812102

2MASS J04062677-3812102 is a main-sequence star of spectral type M4V in the constellation Eridanus, 260.9 light-years from the Sun.

ConstellationEridanus
Distance260.9 light-years (80.0 pc)
Apparent magnitudemagnitude 22.27
Absolute magnitudemagnitude 17.75
Spectral typeM4V
Surface temperature2,980 K
Luminosity1.24 × 10⁻⁴ L☉
Radius0.042 R☉
Mass0.075 M☉ (estimated)
Right ascension (J2000)4h 06m 26.8s
Declination (J2000)−38° 12′ 10″
Space velocity (relative to the Sun)15.0 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 22.27. Visible from the whole Southern Hemisphere and north to latitude 52° N. South of latitude 52° S 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 1765. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 4.6 million years.

The Sun seen from there

From a planet around 2MASS J04062677-3812102, the Sun would look like a star of magnitude 9.35, in the direction where our sky has the constellation Corona Borealis. It would be invisible to the naked eye.

Neighbours

Its nearest neighbours in the catalogue (within 20 light-years):

  • HIP 19775 7.41 light-years
  • HIP 18702 8.84 light-years
  • HIP 18513 10.8 light-years
  • HIP 18857 13.9 light-years
  • HIP 19582 15.8 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.