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Star · G5V

Kepler-150

Kepler-150 is a main-sequence star of spectral type G5V in the constellation Lyra, 2,906 light-years from the Sun. It is orbited by 5 confirmed exoplanet(s).

ConstellationLyra
Distance2,906 light-years (891.1 pc)
Apparent magnitudemagnitude 15.16
Absolute magnitudemagnitude 5.41
Spectral typeG5V
Surface temperature5,560 K
Luminosity0.69 L☉
Radius0.939 R☉
Mass0.956 M☉
Age1.7 billion years
Metallicity [Fe/H]0.12
Right ascension (J2000)19h 12m 56.2s
Declination (J2000)+40° 31′ 15″
Space velocity (relative to the Sun)6.2 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 15.16. Visible from the whole Northern Hemisphere and south to latitude 49° S. North of latitude 49° 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 881 BC. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 52 million years.

The Sun seen from there

From a planet around Kepler-150, the Sun would look like a star of magnitude 14.58, 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.