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Star · M4V

ULAS J152526.25+095814.3

ULAS J152526.25+095814.3 is a main-sequence star of spectral type M4V in the constellation Serpens, 150.0 light-years from the Sun.

ConstellationSerpens
Distance150.0 light-years (46.0 pc)
Apparent magnitudemagnitude 26.04
Absolute magnitudemagnitude 22.73
Spectral typeM4V
Surface temperature2,980 K
Luminosity1.28 × 10⁻⁶ L☉
Radius0.00425 R☉
Mass0.075 M☉ (estimated)
Right ascension (J2000)15h 25m 26.1s
Declination (J2000)+9° 58′ 13″
Space velocity (relative to the Sun)33.3 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 26.04. Visible from the whole Northern Hemisphere and south to latitude 80° S. It stands highest at midnight in May, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1876. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 2.7 million years.

The Sun seen from there

From a planet around ULAS J152526.25+095814.3, the Sun would look like a star of magnitude 8.14, in the direction where our sky has the constellation Eridanus. It would be invisible to the naked eye.

Neighbours

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

  • HIP 74930 8.60 light-years
  • HIP 76543 9.30 light-years
  • HD 136925 11.3 light-years
  • HIP 76912 13.3 light-years
  • HIP 74931 15.0 light-years
  • HIP 77098 16.9 light-years
  • 2MASS J15515237+0941148 17.2 light-years
  • HIP 75971 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.