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Star · M4V

2MASS J12352675+4124310

2MASS J12352675+4124310 is a main-sequence star of spectral type M4V in the constellation Canes Venatici, 212.0 light-years from the Sun.

ConstellationCanes Venatici
Distance212.0 light-years (65.0 pc)
Apparent magnitudemagnitude 22.21
Absolute magnitudemagnitude 18.15
Spectral typeM4V
Surface temperature2,980 K
Luminosity8.67 × 10⁻⁵ L☉
Radius0.035 R☉
Mass0.075 M☉ (estimated)
Right ascension (J2000)12h 35m 26.7s
Declination (J2000)+41° 24′ 31″
Space velocity (relative to the Sun)27.0 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 22.21. Visible from the whole Northern Hemisphere and south to latitude 49° S. North of latitude 49° N it never sets. It stands highest at midnight in March, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1814. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 3.8 million years.

The Sun seen from there

From a planet around 2MASS J12352675+4124310, the Sun would look like a star of magnitude 8.89, 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 61854 5.51 light-years
  • HIP 61010 9.16 light-years
  • HIP 62201 11.4 light-years
  • 9 CVn 13.0 light-years
  • HIP 60286 13.0 light-years
  • HIP 61880 13.1 light-years
  • SDSS J123112.97+405027.9 13.5 light-years
  • HIP 60094 19.2 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.