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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.

Observing Theta Serpentis from your latitude

From mid-northern latitudes (~40°N), Theta Serpentis reaches a maximum altitude of about 54° above the southern horizon and stays above the horizon for about 12h 34m, best placed July - September.

Your latitudeMax altitudeHours above horizon
60°N (≈ Oslo, Helsinki, Anchorage)34°13h 8m
50°N (≈ London, Prague, Vancouver)44°12h 47m
40°N (≈ Madrid, New York, Beijing)54°12h 34m
30°N (≈ Cairo, Houston, Delhi)64°12h 25m
20°N (≈ Honolulu, Mexico City, Mumbai)74°12h 17m
10°N (≈ Chennai, Bangalore, Bangkok)84°12h 11m
(≈ Quito, Nairobi, Singapore)86°12h 5m
20°S (≈ Rio de Janeiro, Antananarivo, Alice Springs)66°11h 53m
35°S (≈ Sydney, Cape Town, Buenos Aires)51°11h 42m
45°S (≈ Christchurch, Hobart, Puerto Montt)41°11h 33m

Altitudes and durations are geometric, computed for each latitude, independent of date. Set your location below for tonight's exact rise, transit, and set times.

Visibility from New York

From New York tonight, Theta Serpentis rises at 06:07 PM, is highest in the sky at 12:24 AM (53° above the horizon), and sets at 06:40 AM.

Altitude
Azimuth
Max Altitude
53.5°
Rises
06:07 PM
Sets
06:40 AM
Transit
12:24 AM
Theta Serpentis: RA 18h 56m 13.18s, Dec +4° 12' 12.90"
Computed for the night of July 13–14, 2026 (New York).