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Star · M4V

ULAS J012906.88+011350.4

ULAS J012906.88+011350.4 is a main-sequence star of spectral type M4V in the constellation Cetus, 199.0 light-years from the Sun.

ConstellationCetus
Distance199.0 light-years (61.0 pc)
Apparent magnitudemagnitude 23.64
Absolute magnitudemagnitude 19.71
Spectral typeM4V
Surface temperature2,980 K
Luminosity2.05 × 10⁻⁵ L☉
Radius0.017 R☉
Mass0.075 M☉ (estimated)
Right ascension (J2000)1h 29m 06.9s
Declination (J2000)+1° 13′ 50″
Space velocity (relative to the Sun)9.4 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 23.64. Visible from the whole Northern Hemisphere and south to latitude 89° S. 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 1827. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 3.5 million years.

The Sun seen from there

From a planet around ULAS J012906.88+011350.4, the Sun would look like a star of magnitude 8.76, 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 6448 7.10 light-years
  • HIP 7840 11.4 light-years
  • 2MASS J01340281+0508125 15.4 light-years
  • HIP 5699 17.3 light-years
  • HIP 8161 19.0 light-years
  • HIP 6572 19.9 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.