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Star · M4V

2MASS J09393548-2448279

2MASS J09393548-2448279 is a main-sequence star of spectral type M4V in the constellation Antlia, 17.4 light-years from the Sun.

ConstellationAntlia
Distance17.4 light-years (5.35 pc)
Apparent magnitudemagnitude 23.48
Absolute magnitudemagnitude 24.84
Spectral typeM4V
Surface temperature2,980 K
Luminosity1.82 × 10⁻⁷ L☉
Radius0.00161 R☉
Mass0.075 M☉ (estimated)
Right ascension (J2000)9h 39m 35.5s
Declination (J2000)−24° 48′ 28″
Space velocity (relative to the Sun)30.2 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 23.48. Visible from the whole Southern Hemisphere and north to latitude 65° N. South of latitude 65° S 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 2009. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 310 thousand years.

The Sun seen from there

From a planet around 2MASS J09393548-2448279, the Sun would look like a star of magnitude 3.47, in the direction where our sky has the constellation Pegasus. 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.