Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Serpens |
Right ascension | 18h 56m 13.18s[1] |
Declination | +04° 12′ 12.9″[1] |
Apparent magnitude (V) | +4.03 (4.62[2] + 4.98[2] + 6.71[3]) |
Characteristics | |
Spectral type | A5V[4] + A5Vn[4] + G1V[5] |
Astrometry | |
θ¹ Ser | |
Parallax (π) | 21.09 ± 2.86 mas[6] |
Distance | approx. 150 ly (approx. 47 pc) |
θ² Ser | |
Parallax (π) | 19.25 ± 3.57 mas[6] |
Distance | approx. 170 ly (approx. 52 pc) |
θ Ser C | |
Parallax (π) | 37.73 ± 0.51 mas[6] |
Distance | 86 ± 1 ly (26.5 ± 0.4 pc) |
Absolute magnitude (MV) | +4.60[7] |
Details[7] | |
θ Ser C | |
Mass | 1.097 M☉ |
Radius | 0.9870 R☉ |
Luminosity | 1.1817 L☉ |
Temperature | 6,067 K |
Metallicity [Fe/H] | −0.09 dex |
Age | 200 Myr |
Other designations | |
θ1 Ser: Alya, θ Ser A, HR 7141, HD 175638, SAO 124068, HIP 92946, WDS 18562+0412A | |
θ2 Ser: θ Ser B, HR 7142, HD 175639, SAO 124070, HIP 92951, WDS 18562+0412B | |
θ Ser C: HD 175726, HIP 92984, WDS 18562+0412C | |
Database references | |
SIMBAD | θ Ser |
θ¹ Ser | |
θ² Ser | |
θ Ser C |
Theta Serpentis (θ Serpentis, abbreviated Theta Ser, θ Ser) is a triple star system in the constellation of Serpens.
It consists of a binary pair designated Theta Serpentis AB and whose two components are designated Theta1 Serpentis or Theta Serpentis A (officially named Alya /ˈæliə/, the traditional name for the entire system)[8][9] and Theta2 Serpentis or Theta Serpentis B, together with a third visual companion Theta Serpentis C.[10]
Based upon parallax measurements obtained during the Hipparcos mission, θ Serpentis AB is approximately 160 light-years, and θ Serpentis C approximately 86 light-years, from the Sun.
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