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Theta Serpentis

4-8 inch Telescope • Challenging Doubles Theta Serpentis finder map.

Finder map for Theta Serpentis

The proper name Alya is thought to derive from an Arabic term associated with a sheep’s tail, reflecting traditional Arabic star nomenclature for this region of the sky. It has no significant mythological role in Western astronomy. Best observed when high in the sky for the most pleasing view, although the wide separation of the components makes the pair accessible under a wide range of observing conditions. The challenge lies not in resolving the pair—which is easy in small telescopes—but in detecting any subtle brightness difference or faint color contrast between the nearly equal white components.

Theta Serpentis finder optic view.

Finder scope & binocular view of Theta Serpentis

PropertyValue
Common namesAlya
Catalog namestet1 Ser
TypeStar
SubtypeDouble Star
Coordinates18h 56m 13.18s, +4° 12’ 12.90”
SeasonJune - August
Best monthJuly
Beginner friendlyMarginal
Visual rewardModerate
Filters requiredNone
LP toleranceHigh
Minimum equipmentMedium telescope
Optimal equipmentMedium telescope
Magnitude4.6
Size-
ConstellationSerpens

Observation Notes

Naked Eye

Visible from moderately light-polluted skies as a single 4th-magnitude star in Serpens Cauda (the Serpent’s Tail). No duplicity is apparent without optical aid.

Binoculars

Appears as a single bright star. Binoculars do not reliably show elongation or separation of the components.

Small Telescope

An excellent and rewarding double-star target. A small telescope in the 60–80 mm range can split the pair at moderate magnification under steady seeing, revealing two nearly equal white stars with a clear separation.

Medium Telescope

Provides a clean, comfortable split with obvious dark space between the components. The slight difference in brightness becomes noticeable, though color contrast remains minimal.

Large Telescope

Resolves the pair effortlessly at a wide range of magnifications, showing two sharp stellar points. No additional components are visible.