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Star · M1

Kepler-186

Kepler-186 is a main-sequence star of spectral type M1 in the constellation Cygnus, 579.2 light-years from the Sun. It is orbited by 5 confirmed exoplanet(s).

ConstellationCygnus
Distance579.2 light-years (177.6 pc)
Apparent magnitudemagnitude 15.14
Absolute magnitudemagnitude 8.89
Spectral typeM1
Surface temperature3,790 K
Luminosity0.0412 L☉
Radius0.472 R☉
Mass0.478 M☉
Age4.0 billion years
Metallicity [Fe/H]-0.28
Right ascension (J2000)19h 54m 36.7s
Declination (J2000)+43° 57′ 18″
Space velocity (relative to the Sun)4.1 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 15.14. Visible from the whole Northern Hemisphere and south to latitude 46° S. North of latitude 46° N it never sets. It stands highest at midnight in July, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1447. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 10 million years.

The Sun seen from there

From a planet around Kepler-186, the Sun would look like a star of magnitude 11.08, in the direction where our sky has the constellation Puppis. It would be invisible to the naked eye.

Planets

Open in the simulation

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