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Star · M4V

CFBDS J214139.77-033739.0

CFBDS J214139.77-033739.0 is a main-sequence star of spectral type M4V in the constellation Aquarius, 192.4 light-years from the Sun.

ConstellationAquarius
Distance192.4 light-years (59.0 pc)
Apparent magnitudemagnitude 27.85
Absolute magnitudemagnitude 24.00
Spectral typeM4V
Surface temperature2,980 K
Luminosity3.96 × 10⁻⁷ L☉
Radius0.00237 R☉
Mass0.075 M☉ (estimated)
Right ascension (J2000)21h 41m 39.7s
Declination (J2000)−3° 37′ 39″
Space velocity (relative to the Sun)14.0 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 27.85. Visible from the whole Southern Hemisphere and north to latitude 86° N. It stands highest at midnight in August, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1834. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 3.4 million years.

The Sun seen from there

From a planet around CFBDS J214139.77-033739.0, the Sun would look like a star of magnitude 8.68, in the direction where our sky has the constellation Sextans. 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.