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Star · M4V

2MASS J13081228+6103486

2MASS J13081228+6103486 is a main-sequence star of spectral type M4V in the constellation Ursa Major, 244.6 light-years from the Sun.

ConstellationUrsa Major
Distance244.6 light-years (75.0 pc)
Apparent magnitudemagnitude 22.17
Absolute magnitudemagnitude 17.79
Spectral typeM4V
Surface temperature2,980 K
Luminosity1.20 × 10⁻⁴ L☉
Radius0.0412 R☉
Mass0.075 M☉ (estimated)
Right ascension (J2000)13h 08m 12.3s
Declination (J2000)+61° 03′ 49″
Space velocity (relative to the Sun)15.0 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 22.17. Visible from the whole Northern Hemisphere and south to latitude 29° S. North of latitude 29° 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 1781. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 4.3 million years.

The Sun seen from there

From a planet around 2MASS J13081228+6103486, the Sun would look like a star of magnitude 9.21, in the direction where our sky has the constellation Tucana. It would be invisible to the naked eye.

Neighbours

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

  • SDSS J130148.19+584104.1 10.8 light-years
  • HIP 65336 12.4 light-years
  • HIP 65756 13.3 light-years
  • HIP 65728 14.4 light-years
  • HIP 61886 15.1 light-years
  • TOI-1823 15.7 light-years
  • HIP 61911 17.0 light-years
  • HIP 65057 17.6 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.