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Star · M3.0V

GJ 687

GJ 687 is a main-sequence star of spectral type M3.0V in the constellation Draco, 14.8 light-years from the Sun. It is orbited by 2 confirmed exoplanet(s).

Other namesGl 687 · HIP 86162
ConstellationDraco
Distance14.8 light-years (4.55 pc)
Apparent magnitudemagnitude 9.15
Absolute magnitudemagnitude 10.86
Spectral typeM3.0V
Surface temperature3,410 K
Luminosity0.0213 L☉
Radius0.418 R☉
Mass0.4 M☉
Metallicity [Fe/H]0.06
Right ascension (J2000)17h 36m 25.9s
Declination (J2000)+68° 20′ 21″
Space velocity (relative to the Sun)40.5 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 9.15. Visible from the whole Northern Hemisphere and south to latitude 22° S. North of latitude 22° N 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 2011. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 263 thousand years.

The Sun seen from there

From a planet around GJ 687, the Sun would look like a star of magnitude 3.12, in the direction where our sky has the constellation Dorado. It would be visible to the naked eye.

Planets

Neighbours

Its nearest neighbours in the catalogue (within 20 light-years):

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Stellar parameters from the NASA Exoplanet Archive; position and brightness from the HYG / AT-HYG catalogue.