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Star · M4V

ULAS J151821.34+085517.5

ULAS J151821.34+085517.5 is a main-sequence star of spectral type M4V in the constellation Serpens, 185.9 light-years from the Sun.

ConstellationSerpens
Distance185.9 light-years (57.0 pc)
Apparent magnitudemagnitude 22.92
Absolute magnitudemagnitude 19.14
Spectral typeM4V
Surface temperature2,980 K
Luminosity3.47 × 10⁻⁵ L☉
Radius0.0222 R☉
Mass0.075 M☉ (estimated)
Right ascension (J2000)15h 18m 21.4s
Declination (J2000)+8° 55′ 18″
Space velocity (relative to the Sun)30.5 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 22.92. Visible from the whole Northern Hemisphere and south to latitude 81° 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 1840. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 3.3 million years.

The Sun seen from there

From a planet around ULAS J151821.34+085517.5, the Sun would look like a star of magnitude 8.61, 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):

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.