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Star · M4V

2MASS J00191296-6226005

2MASS J00191296-6226005 is a main-sequence star of spectral type M4V in the constellation Tucana, 159.8 light-years from the Sun.

ConstellationTucana
Distance159.8 light-years (49.0 pc)
Apparent magnitudemagnitude 21.14
Absolute magnitudemagnitude 17.69
Spectral typeM4V
Surface temperature2,980 K
Luminosity1.32 × 10⁻⁴ L☉
Radius0.0432 R☉
Mass0.075 M☉ (estimated)
Right ascension (J2000)0h 19m 12.9s
Declination (J2000)−62° 26′ 00″
Space velocity (relative to the Sun)24.0 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 21.14. Visible from the whole Southern Hemisphere and north to latitude 28° N. South of latitude 28° S it never sets. It stands highest at midnight in September, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1866. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 2.8 million years.

The Sun seen from there

From a planet around 2MASS J00191296-6226005, the Sun would look like a star of magnitude 8.28, in the direction where our sky has the constellation Ursa Major. 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.