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Star · G0 V

HD 210277

HD 210277 is a main-sequence star of spectral type G0 V in the constellation Aquarius, 69.6 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).

Other namesGl 848.4 · HIP 109378
ConstellationAquarius
Distance69.6 light-years (21.3 pc)
Apparent magnitudemagnitude 6.54
Absolute magnitudemagnitude 4.89
Spectral typeG0 V
Surface temperature5,540 K
Luminosity0.929 L☉
Radius1.07 R☉
Mass1.01 M☉
Age12.0 billion years
Metallicity [Fe/H]0.22
Right ascension (J2000)22h 09m 29.9s
Declination (J2000)−7° 32′ 55″
Space velocity (relative to the Sun)50.8 km/s

In the sky

Too faint for the naked eye (magnitude 6.54); binoculars will find it. Visible from the whole Southern Hemisphere and north to latitude 82° N. It stands highest at midnight in August, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1956. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 1.2 million years.

The Sun seen from there

From a planet around HD 210277, the Sun would look like a star of magnitude 6.48, in the direction where our sky has the constellation Leo. 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.