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Star · M4V

2MASS J18283572-4849046

2MASS J18283572-4849046 is a main-sequence star of spectral type M4V in the constellation Telescopium, 37.1 light-years from the Sun.

ConstellationTelescopium
Distance37.1 light-years (11.4 pc)
Apparent magnitudemagnitude 22.68
Absolute magnitudemagnitude 22.40
Spectral typeM4V
Surface temperature2,980 K
Luminosity1.72 × 10⁻⁶ L☉
Radius0.00494 R☉
Mass0.075 M☉ (estimated)
Right ascension (J2000)18h 28m 35.7s
Declination (J2000)−48° 49′ 04″
Space velocity (relative to the Sun)13.5 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 22.68. Visible from the whole Southern Hemisphere and north to latitude 41° N. South of latitude 41° S it never sets. It stands highest at midnight in June, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1989. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 658 thousand years.

The Sun seen from there

From a planet around 2MASS J18283572-4849046, the Sun would look like a star of magnitude 5.11, in the direction where our sky has the constellation Auriga. 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.