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Delta Serpentis — Double Star in Serpens

HIP 76276; Delta Serpentis; 13 Serpentis

Observable Double Star Excellent (69/100)

Sep: 4.0", Companion: mag 5.2

Magnitude 3.8m DoubleStar Serpens (Ser) Visible
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About Delta Ser

Description

Delta Serpentis is a multiple-star system about 155 light-years away in the head of the celestial serpent. The primary is an F-type subgiant of spectral class F0 IV at magnitude 3.80. A close F-type companion orbits at 4 arcseconds separation, visible in moderate telescopes. A third component is present at wider separation.

Observing Tips

Delta Ser forms part of the head of Serpens, near Beta Ser. The 4-arcsecond double splits cleanly in a 3-inch telescope at 100x — a satisfying pair of matching white-yellow stars. The wider third component is a binocular target. Best observed April through September.

History

Delta Serpentis retains its Bayer designation in current IAU catalogs.

Fun Facts

Serpens is the only constellation formally divided into two parts (Serpens Caput, the head, and Serpens Cauda, the tail) — with Ophiuchus holding the snake in between. Delta Ser is one of the bright stars of the head, providing an anchor for this unusual two-piece constellation.

Observe

1Physical Properties

Magnitude 3.80
Spectral Type F0IV subgiant
Star Color Yellow-white (B-V 0.26)
Distance 155 ly

2Position & Identifiers

RA 15h 34m 48.1s
Dec +10° 32' 15.0"
Constellation Serpens (Ser)
HR 5788
HIP 76276
HD 138918
SAO 101624
Bayer Delta
Flamsteed 13 Ser
Double Cat 9701

3How easy to split?

Primary 3.8 mag Companion 5.2 mag Separation 4.0″
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Telescope Bortle 3 Bortle 4 Bortle 5
80mm refr. Medium+ Medium+ Medium+
150mm Newt. Easy Easy Easy
C8 203mm Easy Easy Easy
Easy Medium Hard Very hard Impossible

Bortle 3 = rural · 4 = outer suburbs · 5 = suburbs

4Visibility

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Best season Apr – Jun (peak: May)

5Multiple Star System Quadruple

Components 4 (quadruple)
Component IDs AB
Separation 4.0″
Companion Mag 5.2
Position Angle 171°
Star Colors A: Yellow-white B: Yellow-white
Discoverer STF1954
ADS 9701, 3168y, a = 5.8432". Binary with HR 5789, blended mag., colors.

Separation over time

Period: 1150.1 y Eccentricity: 0.683 Now: 4.0", PA 171° -0.02" in 5 years
0.00" 1.2" 2.3" 3.5" 4.6" 2025 2030 2035 2040 2045 4.0"

Apparent separation over time, computed from ORB6 orbital elements. Steep curves indicate fast-changing pairs — catch them while they're splittable.

Eyepiece View

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80x Dawes: 1.9″ TFOV: 0.6°
Realistic = true angular size
N E 171°

A: 3.8 · B: 5.2 · Sep: 4.0″ · PA: 171° · N up, E right

Resolved · Rayleigh: 2.3″ · Dawes: 1.9″ · Eff: 2.3″

Explore

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Size Comparison

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Compare Stars

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Spectral Classification

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Hertzsprung-Russell Diagram

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Stellar Lifecycle

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Blackbody Spectrum

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Stellar Absorption Spectrum

Simulated absorption spectrum based on spectral type. Hover over lines to identify elements.

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Stellar Fusion

Discover

15Stellar Notes

0.022".
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Light Travel Time Machine

17

Relativistic Travel

Nearby in the Sky

Other targets within a few degrees — pan your scope a little and keep exploring.

Visibility scores assume a 150 mm Newton at Bortle 4.

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