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70 Ophiuchi — Double Star in Ophiuchus

Observable Double Star Excellent (61/100)

Sep: 6.7", Companion: mag 6.2

Magnitude 4.0m DoubleStar Ophiuchus (Oph) Visible
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About 70 Oph

Description

70 Ophiuchi is a nearby binary of two K-type main-sequence stars (K0 V + K5 V) about 16.6 light-years away. The pair orbits in a markedly eccentric 88-year orbit, swinging between roughly 1.7″ and 6.7″ apart. Combined visual magnitude is 4.03, with the components at 4.2 and 6.0 — bright enough to study without difficulty.

Observing Tips

Currently around 6.7″ separation (near widest), an easy split at 100×. As the orbit tightens through the 2030s the gap will close to about 1.7″ near 2068, becoming a real test of seeing. The yellow-orange colour contrast is subtle but visible against a dark Ophiuchus background.

History

First catalogued as double by William Herschel in 1779. In the late 19th century Thomas See and others claimed to detect orbital perturbations indicating an unseen massive planet — the announcement was sensational but the supposed planet was eventually shown to be an artefact of measurement error, an early cautionary tale in exoplanet hunting.

Fun Facts

70 Oph's K-dwarf components are about 90 % and 70 % the mass of the Sun, with main-sequence lifetimes far longer than the Sun's — both stars will likely still be shining on the main sequence long after the Sun has evolved into a white dwarf.

Observe

1Physical Properties

Magnitude 4.03
Spectral Type K0V
Star Color Orange (B-V 0.86)
Distance 16 ly

2Position & Identifiers

RA 18h 05m 27.3s
Dec +02° 29' 58.0"
Constellation Ophiuchus (Oph)
HR 6752
HIP 88601
HD 165341
SAO 123107
Flamsteed 70 Oph
Double Cat 11046

3How easy to split?

Primary 4.0 mag Companion 6.2 mag Separation 6.7″
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Telescope Bortle 3 Bortle 4 Bortle 5
80mm refr. Easy Easy Easy
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 May – Jul (peak: Jun)

5Multiple Star System 11 components C,D,R,S,T,U,V,Y,Z: optical

Components 11
Component IDs AB
Separation 6.7″
Companion Mag 6.2
Companion Sp K4V
Position Angle 118°
Star Colors A: Orange B: Orange
Discoverer STF2272
AB 4.20 K0V, 5.99 K4V, 88.13y, a = 4.545". B is 6.00V, +1.15(B-V), vsini =<25k/s. Aitken listed 9 additional faint | companions within 180".

Separation over time

Period: 88.4 y Eccentricity: 0.498 Now: 6.7", PA 116° -0.18" in 5 years
0.00" 1.9" 3.9" 5.8" 7.7" 2025 2030 2035 2040 2045 6.7"

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 118°

A: 4.0 · B: 6.2 · Sep: 6.7″ · PA: 118° · N up, E right

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

Explore

7

Size Comparison

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Spectral Classification

10

Hertzsprung-Russell Diagram

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11

Stellar Lifecycle

12

Blackbody Spectrum

13

Stellar Absorption Spectrum

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

14

Stellar Fusion

Discover

15Stellar Notes

ADS 11046AB, 88.13y D, K 3.4k/s, V0 -7.1k/s, asini 1300.
0.198".
16

Light Travel Time Machine

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Relativistic Travel

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