Xi Serpentis

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Xi Serpentis
Observation data
ICRS
)
Constellation Serpens
Right ascension 17h 37m 35.19983s[1]
Declination −15° 23′ 54.7940″[1]
Apparent magnitude (V) 3.54[2]
Characteristics
Spectral type A9 IIIp Sr[3]
U−B color index +0.12[2]
B−V color index +0.27[2]
Distance
105.3 ± 0.6 ly
(32.3 ± 0.2 pc)
Absolute magnitude (MV)+1.00[5]
Semi-amplitude
(K1)
(primary)
19.4 km/s
Details
ξ Ser Aa
Gyr
ξ Ser Ab
Mass0.18[10] M
HR 6561, SAO 160700[11]
Database references
SIMBADdata

Xi Serpentis,

perihelion passage at a distance of 27 ly (8.2 pc) in around 690,000 years.[12]

The inner pair form a single-lined

Ap star with an abnormal abundance of strontium. The primary has around double[7] the mass of the Sun, while its close companion, component Ab,[13] has only 18%[10]
of the Sun's mass.

The third member, component B, is a magnitude 13.0

arc seconds along a position angle of 78° from the inner pair.[13] It has about 27% of the Sun's mass and an estimated orbital period of 14,763 years.[10]

Name

In

Chinese name for ξ Serpentis itself is Tiān Shì Zuǒ Yuán shí (天市左垣十, English: the Tenth Star of Left Wall of Heavenly Market Enclosure), representing the region of Nanhai (南海, lit. meaning southern sea)[15][16]

References