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Star · M4V

ULAS J020336.94-010231.1

ULAS J020336.94-010231.1 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 25.55
Absolute magnitudemagnitude 21.62
Spectral typeM4V
Surface temperature2,980 K
Luminosity3.52 × 10⁻⁶ L☉
Radius0.00706 R☉
Mass0.075 M☉ (estimated)
Right ascension (J2000)2h 03m 37.2s
Declination (J2000)−1° 02′ 30″
Space velocity (relative to the Sun)97.0 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 25.55. Visible from the whole Southern Hemisphere and north to latitude 89° N. 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 J020336.94-010231.1, 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 9591 5.42 light-years
  • SDSS J020333.26-010812.5 6.53 light-years
  • HIP 10449 9.70 light-years
  • HIP 10033 12.3 light-years
  • HIP 10412 12.9 light-years
  • HIP 9946 16.9 light-years
  • ξ Psc 17.2 light-years
  • HIP 9156 18.1 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.