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Star · M4V

ULAS J235204.62+124444.9

ULAS J235204.62+124444.9 is a main-sequence star of spectral type M4V in the constellation Pegasus, 146.8 light-years from the Sun.

ConstellationPegasus
Distance146.8 light-years (45.0 pc)
Apparent magnitudemagnitude 25.77
Absolute magnitudemagnitude 22.50
Spectral typeM4V
Surface temperature2,980 K
Luminosity1.56 × 10⁻⁶ L☉
Radius0.00471 R☉
Mass0.075 M☉ (estimated)
Right ascension (J2000)23h 52m 04.6s
Declination (J2000)+12° 44′ 47″
Space velocity (relative to the Sun)34.4 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 25.77. Visible from the whole Northern Hemisphere and south to latitude 77° S. North of latitude 77° N it never sets. It stands highest at midnight in September, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1879. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 2.6 million years.

The Sun seen from there

From a planet around ULAS J235204.62+124444.9, the Sun would look like a star of magnitude 8.10, in the direction where our sky has the constellation Crater. It would be invisible to the naked eye.

Neighbours

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

  • HIP 116907 9.48 light-years
  • HIP 117236 10.8 light-years
  • HIP 117235 11.8 light-years
  • HIP 117461 12.3 light-years
  • HIP 117846 12.4 light-years
  • PSO J353.6355+13.2209 12.6 light-years
  • HIP 999 13.7 light-years
  • 2MASS J00133470+1109403 15.8 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.