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Star · M4V

ULAS J015144.10+134645.8

ULAS J015144.10+134645.8 is a main-sequence star of spectral type M4V in the constellation Aries, 228.3 light-years from the Sun.

ConstellationAries
Distance228.3 light-years (70.0 pc)
Apparent magnitudemagnitude 23.16
Absolute magnitudemagnitude 18.93
Spectral typeM4V
Surface temperature2,980 K
Luminosity4.19 × 10⁻⁵ L☉
Radius0.0244 R☉
Mass0.075 M☉ (estimated)
Right ascension (J2000)1h 51m 44.1s
Declination (J2000)+13° 46′ 45″
Space velocity (relative to the Sun)5.7 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 23.16. Visible from the whole Northern Hemisphere and south to latitude 76° S. North of latitude 76° N it never sets. It stands highest at midnight in October, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1798. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 4.1 million years.

The Sun seen from there

From a planet around ULAS J015144.10+134645.8, the Sun would look like a star of magnitude 9.06, in the direction where our sky has the constellation Virgo. It would be invisible to the naked eye.

Neighbours

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

  • HIP 9180 6.29 light-years
  • HIP 9643 14.2 light-years
  • HIP 8872 16.0 light-years
  • HIP 9434 17.4 light-years
  • HIP 9137 17.5 light-years
  • SDSS J021128.25+141003.8 19.1 light-years
  • HIP 8033 19.4 light-years
  • HIP 8110 19.8 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.