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Rasalhague — Double Star in Ophiuchus

HIP 86032; Alpha Ophiuchi; 55 Ophiuchi

Magnitude 2.1m DoubleStar Ophiuchus (Oph) Visible
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About Rasalhague

Description

Rasalhague is a white giant of spectral type A5III at magnitude 2.08, the brightest star in Ophiuchus. Located about 47 light-years from Earth, it has a luminosity of roughly 25 times solar. It is a binary system with a faint companion. Rasalhague is one of the nearest A-type giant stars to the Sun.

Observing Tips

Rasalhague marks the head of Ophiuchus (the Serpent Bearer), forming the northern apex of the large, sprawling constellation. It sits between Hercules to the north and the rich Milky Way star fields of Scorpius to the south. Best observed June through September.

History

The name Rasalhague comes from the Arabic 'ra's al-hawwa,' meaning 'the head of the serpent collector.' Ophiuchus is the unofficial 13th zodiacal constellation, as the ecliptic passes through it between Scorpius and Sagittarius. The constellation represents Asclepius, the Greek god of medicine.

Fun Facts

Rasalhague is only 47 light-years away, making it one of the nearest giant stars to the Sun. The Sun passes through Ophiuchus from November 30 to December 18 each year, making Ophiuchus an unofficial zodiac sign — but astrologers traditionally ignore it.

Observe

1Physical Properties

Magnitude 2.08
Variable Type Delta Scuti (Pulsating)
Spectral Type A5IVnn supergiant
Star Color Yellow-white (B-V 0.15)
Distance 49 ly

2Position & Identifiers

RA 17h 34m 56.1s
Dec +12° 33' 36.0"
Constellation Ophiuchus (Oph)
HR 6556
HIP 86032
HD 159561
SAO 102932
Bayer Alpha
Flamsteed 55 Oph

3How easy to split?

Primary 2.1 mag Companion 5.0 mag Separation 0.8″
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Telescope Bortle 3 Bortle 4 Bortle 5
80mm refr. V. hard V. hard V. hard
150mm Newt. V. hard+ V. hard+ V. hard+
C8 203mm V. hard+ V. hard+ V. hard+
Easy Medium Hard Very hard Impossible

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

To reach "Medium" at Bortle 3, you'd need at least a 420 mm reflector.

4Visibility

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Best season May – Jul (peak: Jun)

5Multiple Star System

Separation 0.8″
Companion Mag 5.0
Position Angle 248°
Star Colors A: Yellow-white
Discoverer MCY 4
A* 2.08 A5III, 8.5y, a = 0.065". Resolved by speckle interferometry.

Separation over time

Period: 8.6 y Eccentricity: 0.939 Now: 0.75", PA 240° -0.14" in 5 years
0.00" 0.23" 0.45" 0.68" 0.91" 2024 2026 2028 2030 0.75"

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 248°

A: 2.1 · B: 5.0 · Sep: 0.8″ · PA: 248° · N up, E right

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

Explore

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Size Comparison

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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

Delta Sct?
UMa stream; Sirius group.
Interstellar CaII lines indicate a cloud of about 1 pc depth in front of Alpha Oph.
RASALHAGUE; Ras Alhague.
Diam. = 0.00153 - 0.00163".
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Light Travel Time Machine

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Relativistic Travel

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