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Star · M4V

ULAS J101243.54+102101.7

ULAS J101243.54+102101.7 is a main-sequence star of spectral type M4V in the constellation Leo, 54.8 light-years from the Sun.

ConstellationLeo
Distance54.8 light-years (16.8 pc)
Apparent magnitudemagnitude 24.38
Absolute magnitudemagnitude 23.25
Spectral typeM4V
Surface temperature2,980 K
Luminosity7.85 × 10⁻⁷ L☉
Radius0.00333 R☉
Mass0.075 M☉ (estimated)
Right ascension (J2000)10h 12m 43.8s
Declination (J2000)+10° 21′ 05″
Space velocity (relative to the Sun)53.4 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 24.38. Visible from the whole Northern Hemisphere and south to latitude 80° S. North of latitude 80° N it never sets. It stands highest at midnight in February, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1971. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 972 thousand years.

The Sun seen from there

From a planet around ULAS J101243.54+102101.7, the Sun would look like a star of magnitude 5.96, in the direction where our sky has the constellation Aquarius. It would be visible 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.