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Star · M4V

ULAS J014927.09+144108.2

ULAS J014927.09+144108.2 is a main-sequence star of spectral type M4V in the constellation Aries, 208.7 light-years from the Sun.

ConstellationAries
Distance208.7 light-years (64.0 pc)
Apparent magnitudemagnitude 23.59
Absolute magnitudemagnitude 19.56
Spectral typeM4V
Surface temperature2,980 K
Luminosity2.36 × 10⁻⁵ L☉
Radius0.0183 R☉
Mass0.075 M☉ (estimated)
Right ascension (J2000)1h 49m 27.1s
Declination (J2000)+14° 41′ 09″
Space velocity (relative to the Sun)12.4 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 23.59. Visible from the whole Northern Hemisphere and south to latitude 75° S. North of latitude 75° 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 1817. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 3.7 million years.

The Sun seen from there

From a planet around ULAS J014927.09+144108.2, the Sun would look like a star of magnitude 8.86, 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 9137 8.09 light-years
  • HIP 9434 15.6 light-years
  • HIP 7447 15.9 light-years
  • HIP 7172 16.2 light-years
  • ULAS J020047.44+133755.1 16.7 light-years
  • HIP 9643 17.6 light-years
  • HIP 9016 18.1 light-years
  • HIP 8033 18.3 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.