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Star · M4V

ULAS J112059.41+121904.5

ULAS J112059.41+121904.5 is a main-sequence star of spectral type M4V in the constellation Leo, 130.5 light-years from the Sun.

ConstellationLeo
Distance130.5 light-years (40.0 pc)
Apparent magnitudemagnitude 25.43
Absolute magnitudemagnitude 22.42
Spectral typeM4V
Surface temperature2,980 K
Luminosity1.69 × 10⁻⁶ L☉
Radius0.00489 R☉
Mass0.075 M☉ (estimated)
Right ascension (J2000)11h 20m 59.5s
Declination (J2000)+12° 19′ 04″
Space velocity (relative to the Sun)10.8 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 25.43. Visible from the whole Northern Hemisphere and south to latitude 78° S. North of latitude 78° 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 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 J112059.41+121904.5, the Sun would look like a star of magnitude 7.84, in the direction where our sky has the constellation Aquarius. It would be invisible to the naked eye.

Neighbours

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

  • HIP 54299 9.43 light-years
  • K2-18 13.2 light-years
  • HIP 56999 13.8 light-years
  • HIP 55605 15.2 light-years
  • HIP 55922 15.6 light-years
  • HIP 54100 15.8 light-years
  • SDSS J110443.47+162435.6 15.8 light-years
  • HIP 54553 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.