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Star · G5V

Kepler-865

Kepler-865 is a main-sequence star of spectral type G5V in the constellation Cygnus, 1,912 light-years from the Sun. It is orbited by 2 confirmed exoplanet(s).

ConstellationCygnus
Distance1,912 light-years (586.1 pc)
Apparent magnitudemagnitude 14.64
Absolute magnitudemagnitude 5.80
Spectral typeG5V
Surface temperature5,570 K
Luminosity0.504 L☉
Radius0.92 R☉
Mass0.93 M☉
Age4.3 billion years
Metallicity [Fe/H]-0.01
Right ascension (J2000)19h 50m 53.8s
Declination (J2000)+43° 31′ 38″
Space velocity (relative to the Sun)102.4 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 14.64. 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 114. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 34 million years.

The Sun seen from there

From a planet around Kepler-865, the Sun would look like a star of magnitude 13.67, 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.