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Star · M4V

ULAS J130444.26+310112.3

ULAS J130444.26+310112.3 is a main-sequence star of spectral type M4V in the constellation Coma Berenices, 137.0 light-years from the Sun.

ConstellationComa Berenices
Distance137.0 light-years (42.0 pc)
Apparent magnitudemagnitude 26.29
Absolute magnitudemagnitude 23.17
Spectral typeM4V
Surface temperature2,980 K
Luminosity8.44 × 10⁻⁷ L☉
Radius0.00346 R☉
Mass0.075 M☉ (estimated)
Right ascension (J2000)13h 04m 44.3s
Declination (J2000)+31° 01′ 12″
Space velocity (relative to the Sun)6.0 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 26.29. Visible from the whole Northern Hemisphere and south to latitude 59° S. North of latitude 59° 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 1889. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 2.4 million years.

The Sun seen from there

From a planet around ULAS J130444.26+310112.3, the Sun would look like a star of magnitude 7.95, 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 63048 9.97 light-years
  • HIP 64761 12.2 light-years
  • HIP 64131 12.9 light-years
  • HIP 65706 13.1 light-years
  • HIP 61739 14.0 light-years
  • HIP 62181 14.3 light-years
  • HIP 62739 15.7 light-years
  • HIP 63181 16.5 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.