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Star · M4V

ULAS J131304.03+225919.7

ULAS J131304.03+225919.7 is a main-sequence star of spectral type M4V in the constellation Coma Berenices, 130.5 light-years from the Sun.

ConstellationComa Berenices
Distance130.5 light-years (40.0 pc)
Apparent magnitudemagnitude 25.41
Absolute magnitudemagnitude 22.40
Spectral typeM4V
Surface temperature2,980 K
Luminosity1.72 × 10⁻⁶ L☉
Radius0.00494 R☉
Mass0.075 M☉ (estimated)
Right ascension (J2000)13h 13m 03.8s
Declination (J2000)+22° 59′ 20″
Space velocity (relative to the Sun)35.6 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 25.41. Visible from the whole Northern Hemisphere and south to latitude 67° S. North of latitude 67° 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 1896. 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 ULAS J131304.03+225919.7, the Sun would look like a star of magnitude 7.84, in the direction where our sky has the constellation Cetus. It would be invisible to the naked eye.

Neighbours

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

  • HIP 64059 9.04 light-years
  • HIP 64057 9.24 light-years
  • HIP 66072 10.7 light-years
  • HIP 64761 10.9 light-years
  • HIP 62772 11.4 light-years
  • HIP 62794 12.4 light-years
  • HIP 63497 12.6 light-years
  • HIP 62758 13.1 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.