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Star · M2V

SIPS J0614-2019

SIPS J0614-2019 is a main-sequence star of spectral type M2V in the constellation Canis Major, 100.5 light-years from the Sun.

ConstellationCanis Major
Distance100.5 light-years (30.8 pc)
Apparent magnitudemagnitude 21.52
Absolute magnitudemagnitude 19.08
Spectral typeM2V
Surface temperature3,300 K
Luminosity1.67 × 10⁻⁵ L☉
Radius0.0125 R☉
Mass0.075 M☉ (estimated)
Right ascension (J2000)6h 14m 12.1s
Declination (J2000)−20° 19′ 23″
Space velocity (relative to the Sun)49.3 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 21.52. Visible from the whole Southern Hemisphere and north to latitude 70° N. South of latitude 70° S it never sets. 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 1925. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 1.8 million years.

The Sun seen from there

From a planet around SIPS J0614-2019, the Sun would look like a star of magnitude 7.27, in the direction where our sky has the constellation Hercules. 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.