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Star · M4V

2MASS J13120707+3937445

2MASS J13120707+3937445 is a main-sequence star of spectral type M4V in the constellation Canes Venatici, 159.8 light-years from the Sun.

ConstellationCanes Venatici
Distance159.8 light-years (49.0 pc)
Apparent magnitudemagnitude 19.67
Absolute magnitudemagnitude 16.22
Spectral typeM4V
Surface temperature2,980 K
Luminosity5.11 × 10⁻⁴ L☉
Radius0.0851 R☉
Mass0.075 M☉ (estimated)
Right ascension (J2000)13h 12m 07.1s
Declination (J2000)+39° 37′ 44″
Space velocity (relative to the Sun)25.7 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 19.67. Visible from the whole Northern Hemisphere and south to latitude 50° S. North of latitude 50° 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 1866. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 2.8 million years.

The Sun seen from there

From a planet around 2MASS J13120707+3937445, the Sun would look like a star of magnitude 8.28, in the direction where our sky has the constellation Phoenix. It would be invisible to the naked eye.

Neighbours

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

  • HIP 65049 5.95 light-years
  • HIP 65485 11.0 light-years
  • HIP 64747 12.3 light-years
  • HIP 65937 13.9 light-years
  • HIP 66257 15.5 light-years
  • HIP 64134 16.4 light-years
  • HIP 65935 16.9 light-years
  • HIP 65135 17.3 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.