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Star · M4V

ULAS J002740.95+085940.3

ULAS J002740.95+085940.3 is a main-sequence star of spectral type M4V in the constellation Pisces, 228.3 light-years from the Sun.

ConstellationPisces
Distance228.3 light-years (70.0 pc)
Apparent magnitudemagnitude 25.70
Absolute magnitudemagnitude 21.47
Spectral typeM4V
Surface temperature2,980 K
Luminosity4.04 × 10⁻⁶ L☉
Radius0.00756 R☉
Mass0.075 M☉ (estimated)
Right ascension (J2000)0h 27m 40.8s
Declination (J2000)+8° 59′ 46″
Space velocity (relative to the Sun)117.1 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 25.70. Visible from the whole Northern Hemisphere and south to latitude 81° S. 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 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 J002740.95+085940.3, 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 2751 9.95 light-years
  • HIP 2724 14.1 light-years
  • HIP 2358 16.6 light-years
  • 35 Psc 17.4 light-years
  • HIP 795 17.7 light-years
  • HIP 3033 18.4 light-years
  • HIP 1197 19.1 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.