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Star · G2 V

HD 222155

HD 222155 is a main-sequence star of spectral type G2 V in the constellation Andromeda, 164.7 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).

Other namesHIP 116616
ConstellationAndromeda
Distance164.7 light-years (50.5 pc)
Apparent magnitudemagnitude 7.11
Absolute magnitudemagnitude 3.59
Spectral typeG2 V
Surface temperature5,700 K
Luminosity3.23 L☉
Radius1.85 R☉
Mass1.21 M☉
Age8.2 billion years
Metallicity [Fe/H]-0.18
Right ascension (J2000)23h 38m 00.3s
Declination (J2000)+48° 59′ 48″
Space velocity (relative to the Sun)70.1 km/s

In the sky

Too faint for the naked eye (magnitude 7.11); binoculars will find it. Visible from the whole Northern Hemisphere and south to latitude 41° S. North of latitude 41° N 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 1861. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 2.9 million years.

The Sun seen from there

From a planet around HD 222155, the Sun would look like a star of magnitude 8.35, in the direction where our sky has the constellation Centaurus. 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.