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Star · K

Kepler-444

Kepler-444 is a main-sequence star of spectral type K in the constellation Lyra, 119.2 light-years from the Sun. It is orbited by 5 confirmed exoplanet(s).

Other namesHIP 94931
ConstellationLyra
Distance119.2 light-years (36.6 pc)
Apparent magnitudemagnitude 8.87
Absolute magnitudemagnitude 6.06
Spectral typeK
Surface temperature5,050 K
Luminosity0.376 L☉
Radius0.752 R☉
Mass0.758 M☉
Age11.2 billion years
Metallicity [Fe/H]-0.55
Right ascension (J2000)19h 19m 00.6s
Declination (J2000)+41° 38′ 05″
Space velocity (relative to the Sun)163.9 km/s

In the sky

Too faint for the naked eye (magnitude 8.87); binoculars will find it. Visible from the whole Northern Hemisphere and south to latitude 48° S. North of latitude 48° 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 1907. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 2.1 million years.

The Sun seen from there

From a planet around Kepler-444, the Sun would look like a star of magnitude 7.64, in the direction where our sky has the constellation Puppis. It would be invisible 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.