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Star · M4V

SDSS J102552.43+321234.0

SDSS J102552.43+321234.0 is a main-sequence star of spectral type M4V in the constellation Leo Minor, 87.4 light-years from the Sun.

ConstellationLeo Minor
Distance87.4 light-years (26.8 pc)
Apparent magnitudemagnitude 22.54
Absolute magnitudemagnitude 20.40
Spectral typeM4V
Surface temperature2,980 K
Luminosity1.09 × 10⁻⁵ L☉
Radius0.0124 R☉
Mass0.075 M☉ (estimated)
Right ascension (J2000)10h 25m 52.3s
Declination (J2000)+32° 12′ 35″
Space velocity (relative to the Sun)49.7 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 22.54. Visible from the whole Northern Hemisphere and south to latitude 58° S. North of latitude 58° 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 1939. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 1.6 million years.

The Sun seen from there

From a planet around SDSS J102552.43+321234.0, the Sun would look like a star of magnitude 6.97, in the direction where our sky has the constellation Piscis Austrinus. 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.