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Star · M4V

WISEA J131845.58+362614.0

WISEA J131845.58+362614.0 is a main-sequence star of spectral type M4V in the constellation Canes Venatici, 127.2 light-years from the Sun.

ConstellationCanes Venatici
Distance127.2 light-years (39.0 pc)
Apparent magnitudemagnitude 22.71
Absolute magnitudemagnitude 19.75
Spectral typeM4V
Surface temperature2,980 K
Luminosity1.97 × 10⁻⁵ L☉
Radius0.0167 R☉
Mass0.075 M☉ (estimated)
Right ascension (J2000)13h 18m 45.7s
Declination (J2000)+36° 26′ 14″
Space velocity (relative to the Sun)20.9 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 22.71. Visible from the whole Northern Hemisphere and south to latitude 54° S. North of latitude 54° 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 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 WISEA J131845.58+362614.0, the Sun would look like a star of magnitude 7.79, in the direction where our sky has the constellation Sculptor. It would be invisible to the naked eye.

Neighbours

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

  • HIP 66194 8.85 light-years
  • HIP 63181 10.0 light-years
  • HIP 63317 11.8 light-years
  • HIP 63322 13.0 light-years
  • TOI-1807 13.4 light-years
  • HIP 63303 14.1 light-years
  • HIP 65775 14.5 light-years
  • HIP 66593 15.3 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.