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Star · M4V

Ross 614

Ross 614 is a main-sequence star of spectral type M4V in the constellation Monoceros, 13.4 light-years from the Sun.

Other namesGl 234A · HIP 30920
ConstellationMonoceros
Distance13.4 light-years (4.12 pc)
Apparent magnitudemagnitude 11.12
Absolute magnitudemagnitude 13.05
Spectral typeM4V
Surface temperature3,530 K
Luminosity0.00283 L☉
Radius0.142 R☉
Mass0.148 M☉ (estimated)
Right ascension (J2000)6h 29m 23.0s
Declination (J2000)−2° 48′ 47″
Space velocity (relative to the Sun)27.1 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 11.12. Visible from the whole Southern Hemisphere and north to latitude 87° N. It stands highest at midnight in December, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 2013. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 238 thousand years.

The Sun seen from there

From a planet around Ross 614, the Sun would look like a star of magnitude 2.90, in the direction where our sky has the constellation Serpens. 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.