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Star · K3 V

HD 222237

HD 222237 is a main-sequence star of spectral type K3 V in the constellation Tucana, 37.3 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).

Other namesGl 902 · HIP 116745
ConstellationTucana
Distance37.3 light-years (11.4 pc)
Apparent magnitudemagnitude 7.09
Absolute magnitudemagnitude 6.80
Spectral typeK3 V
Surface temperature4,750 K
Luminosity0.216 L☉
Radius0.71 R☉
Mass0.76 M☉
Age8.8 billion years
Metallicity [Fe/H]-0.32
Right ascension (J2000)23h 39m 37.1s
Declination (J2000)−72° 43′ 19″
Space velocity (relative to the Sun)80.7 km/s

In the sky

Too faint for the naked eye (magnitude 7.09); binoculars will find it. Visible from the whole Southern Hemisphere and north to latitude 17° N. South of latitude 17° S it never sets. It stands highest at midnight in September, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1989. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 662 thousand years.

The Sun seen from there

From a planet around HD 222237, the Sun would look like a star of magnitude 5.12, in the direction where our sky has the constellation Draco. 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.