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Star · M3V

SDSS J104842.84+011158.5

SDSS J104842.84+011158.5 is a main-sequence star of spectral type M3V in the constellation Sextans, 49.0 light-years from the Sun.

ConstellationSextans
Distance49.0 light-years (15.0 pc)
Apparent magnitudemagnitude 20.73
Absolute magnitudemagnitude 19.85
Spectral typeM3V
Surface temperature3,070 K
Luminosity1.41 × 10⁻⁵ L☉
Radius0.0133 R☉
Mass0.075 M☉ (estimated)
Right ascension (J2000)10h 48m 42.3s
Declination (J2000)+1° 11′ 55″
Space velocity (relative to the Sun)35.4 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 20.73. Visible from the whole Northern Hemisphere and south to latitude 89° S. It stands highest at midnight in March, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1977. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 869 thousand years.

The Sun seen from there

From a planet around SDSS J104842.84+011158.5, the Sun would look like a star of magnitude 5.71, 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.