Star Zeta Serpentis
Yellow-White star Zeta Serpentis is located 75 light years away from the Sun.
It is a single star of spectral class F2V, that has 143 % of solar mass.
For now, there are no known exoplanets in this star system.
More about Zeta Serpentis
Nearby star Zeta Serpentis is a main sequence star that fuses hydrogen atoms into helium. It is is approximately 96 % bigger than the Sun and temperature on its surface is around 6529 K (6256 °C), which is about 113 % of Sun's temperature.
Zeta Serpentis can be found in southern celestial hemisphere, and it is possible to see it with naked eye. The star is also observable from Northern America, Europe and Asia.
Other designations of this star
ζ Ser, 57 Serpentis, BD−03° 4217, GC 24503, HD 164259, HIP 88175, HR 6710, SAO 142025, Gaia EDR3 4177224620176470912
External sources
Simbad database (* zet Ser)
Astronomical database SIMBAD (the Set of Identifications, Measurements and Bibliography for Astronomical Data)
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Right ascension: 18h 0m 29.18s
Declination: -3° 41' 25.712'' (equatorial region)
Parallax: 43.482
Sun distance: 75.009 ly | 23 pc
Temperature: 6529 K | 1.13 T Sun
Age: 2.4 billions years | 0.52 Sun
Luminosity: 6.251 L Sun
Apparent magnitude (V): 4.6
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