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Star · G8 III

ω Ser

ω Ser is a giant star of spectral type G8 III in the constellation Serpens, 248.9 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).

Other namesome Ser · HIP 77578
ConstellationSerpens
Distance248.9 light-years (76.3 pc)
Apparent magnitudemagnitude 5.21
Absolute magnitudemagnitude 0.80
Spectral typeG8 III
Surface temperature4,720 K
Luminosity54.2 L☉
Radius11 R☉
Mass1.01 M☉
Metallicity [Fe/H]-0.12
Right ascension (J2000)15h 50m 17.5s
Declination (J2000)+2° 11′ 48″
Space velocity (relative to the Sun)20.8 km/s

In the sky

Visible to the naked eye under a dark sky (apparent magnitude 5.21). Visible from the whole Northern Hemisphere and south to latitude 88° S. It stands highest at midnight in May, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1777. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 4.4 million years.

The Sun seen from there

From a planet around ω Ser, the Sun would look like a star of magnitude 9.24, in the direction where our sky has the constellation Eridanus. 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.