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Ascella — Double Star in Sagittarius

HIP 93506; Zeta Sagittarii; 38 Sagittarii

Magnitude 2.6m DoubleStar Sagittarius (Sgr) Visible
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About Ascella

Description

Ascella is a white binary star of spectral type A2III+A4IV at magnitude 2.60 in Sagittarius. Located about 89 light-years from Earth, it consists of two A-type stars orbiting each other every 21 years. Ascella forms the base or 'armpit' of the Archer figure and part of the Teapot handle.

Observing Tips

Ascella sits at the bottom of the Teapot handle in Sagittarius. The two components can be resolved in a moderate telescope when near maximum separation. It is a warm white star in the rich Milky Way fields. Best observed July through September.

History

The name Ascella comes from the Latin 'ascella,' meaning 'the armpit,' referring to its position under the Archer's arm. As a relatively nearby bright binary, it has been well-studied since the discovery of its double nature.

Fun Facts

Ascella's two A-type components make it a true physical binary — both stars formed together and orbit their common center of mass. The 21-year orbital period is short enough that the system's orbital motion has been well characterized over decades of observation.

Observe

1Physical Properties

Magnitude 2.60
Spectral Type A2.5Va
Star Color White (B-V 0.08)
Distance 88 ly

2Position & Identifiers

RA 19h 02m 36.7s
Dec -29° 52' 49.0"
Constellation Sagittarius (Sgr)
HR 7194
HIP 93506
HD 176687
SAO 187600
Bayer Zeta
Flamsteed 38 Sgr
Double Cat 11950

3How easy to split?

Primary 2.6 mag Companion 3.5 mag Separation 0.4″
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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 580 mm reflector.

4Visibility

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Best season Jun – Aug (peak: Jul)

5Multiple Star System Triple

Components 3 (triple)
Component IDs AB
Separation 0.4″
Companion Mag 3.5
Companion Sp A4
Position Angle 133°
Star Colors A: White B: White
Discoverer HDO 150
AB 3.2 A2III, 3.4 A2V, 21.138y, a = 0.532".

Separation over time

Period: 21.0 y Eccentricity: 0.211 Now: 0.39", PA 77° -0.16" in 5 years
0.00" 0.17" 0.34" 0.51" 0.68" 2016 2020 2024 2028 2032 2036 0.39"

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 133°

A: 2.6 · B: 3.5 · Sep: 0.4″ · PA: 133° · 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

0.040".
Ascella.
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Light Travel Time Machine

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Relativistic Travel

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