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Star · M3V

SDSSp J053951.99-005902.0

SDSSp J053951.99-005902.0 is a main-sequence star of spectral type M3V in the constellation Orion, 41.3 light-years from the Sun.

ConstellationOrion
Distance41.3 light-years (12.7 pc)
Apparent magnitudemagnitude 21.79
Absolute magnitudemagnitude 21.28
Spectral typeM3V
Surface temperature3,130 K
Luminosity3.23 × 10⁻⁶ L☉
Radius0.0061 R☉
Mass0.075 M☉ (estimated)
Right ascension (J2000)5h 39m 52.2s
Declination (J2000)−0° 58′ 56″
Space velocity (relative to the Sun)25.8 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 21.79. Visible from the whole Southern Hemisphere and north to latitude 89° N. It stands highest at midnight in December, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1985. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 733 thousand years.

The Sun seen from there

From a planet around SDSSp J053951.99-005902.0, the Sun would look like a star of magnitude 5.34, in the direction where our sky has the constellation Ophiuchus. 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.