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Star · M4V

ULAS J154701.84+005320.3

ULAS J154701.84+005320.3 is a main-sequence star of spectral type M4V in the constellation Serpens, 127.2 light-years from the Sun.

ConstellationSerpens
Distance127.2 light-years (39.0 pc)
Apparent magnitudemagnitude 25.82
Absolute magnitudemagnitude 22.86
Spectral typeM4V
Surface temperature2,980 K
Luminosity1.12 × 10⁻⁶ L☉
Radius0.00399 R☉
Mass0.075 M☉ (estimated)
Right ascension (J2000)15h 47m 01.8s
Declination (J2000)+0° 53′ 21″
Space velocity (relative to the Sun)14.1 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 25.82. Visible from the whole Northern Hemisphere and south to latitude 89° 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 1899. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 2.3 million years.

The Sun seen from there

From a planet around ULAS J154701.84+005320.3, the Sun would look like a star of magnitude 7.79, 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.