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Star · F6V

γ Ser

γ Ser is a main-sequence star of spectral type F6V in the constellation Serpens, 36.4 light-years from the Sun.

Other namesGl 603 · HIP 78072
ConstellationSerpens
Distance36.4 light-years (11.2 pc)
Apparent magnitudemagnitude 3.85
Absolute magnitudemagnitude 3.61
Spectral typeF6V
Surface temperature6,490 K
Luminosity3.08 L☉
Radius1.39 R☉
Mass1.32 M☉ (estimated)
Right ascension (J2000)15h 56m 27.2s
Declination (J2000)+15° 39′ 42″
Space velocity (relative to the Sun)70.1 km/s

In the sky

Visible to the naked eye under a dark sky (apparent magnitude 3.85). Visible from the whole Northern Hemisphere and south to latitude 74° S. North of latitude 74° N it never sets. 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 1990. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 646 thousand years.

The Sun seen from there

From a planet around γ Ser, the Sun would look like a star of magnitude 5.07, in the direction where our sky has the constellation Eridanus. It would be visible to the naked eye.

Neighbours

Its nearest neighbours in the catalogue (within 20 light-years):

Open in the simulation

Position, brightness and colour from the HYG / AT-HYG catalogue; temperature, luminosity, radius and mass are approximate values computed from these observations.