Alya (star)

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θ1 Serpentis (θ Serpentis A) ("Alya")
Imperiumgrey-2.jpg
Spectral A5 V
Type Main Sequence
Multiple Binary
Luminosity 33 LSol
Absolute magnitude
Mag Terra 4.62
Temperature 8000° K
Mass 2.2 MSol
Radius 3.3 RSol
Companion θ2 Serpentis
θ2 Serpentis (θ Serpentis B)
Imperiumgrey-2.jpg
Spectral A5 Vn
Type Main Sequence
Multiple Companion
Luminosity 24 LSol
Absolute magnitude
Mag Terra 4.98
Temperature 8000° K
Mass 2.0 MSol
Radius 2.9 RSol
Companion θ1 Serpentis

The star Theta Serpentis (θ Serpentis) (whose A-component is otherwise known as Alya) is a binary star system composed of two bluish-white main sequence stars of spectral type A5.

Description (Specifications)[edit]

The θ1 and θ2 components of this star system lie approximately 900AU from one another, yielding a mutual orbital period of about 14000 years.

  • A third G5 V star known to ancient Solomani astronomers as θ Serpentis C is merely a line-of-sight optical companion of the θ12 Serpentis system from the vantage point of a Terran-based observer, and is not actually a member of this star system.

History & Background (Dossier)[edit]

The Alya star system lies approximately 40pc from Terra, and is located in a Coreward/Corespinward direction from Terra at bearing 037.2o Galactic Longitude and +00.9o North Galactic Latitude.

References & Contributors (Sources)[edit]

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