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Star · G2V

HD 168009

HD 168009 is a main-sequence star of spectral type G2V in the constellation Lyra, 76.0 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).

Other namesGl 708.4 · HIP 89474
ConstellationLyra
Distance76.0 light-years (23.3 pc)
Apparent magnitudemagnitude 6.30
Absolute magnitudemagnitude 4.46
Spectral typeG2V
Surface temperature5,780 K
Luminosity1.41 L☉
Radius1.21 R☉
Mass0.986 M☉
Age9.7 billion years
Metallicity [Fe/H]0.02
Right ascension (J2000)18h 15m 32.5s
Declination (J2000)+45° 12′ 34″
Space velocity (relative to the Sun)66.3 km/s

In the sky

Visible to the naked eye under a dark sky (apparent magnitude 6.30). Visible from the whole Northern Hemisphere and south to latitude 45° S. North of latitude 45° N it never sets. It stands highest at midnight in June, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1950. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 1.3 million years.

The Sun seen from there

From a planet around HD 168009, the Sun would look like a star of magnitude 6.67, 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.