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Dschubba — Double Star in Scorpius

HIP 78401; Delta Scorpii; 7 Scorpii

Magnitude 2.3m DoubleStar Scorpius (Sco) Visible
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About Dschubba

Description

Dschubba is a blue subgiant of spectral type B0.3IV at magnitude 2.32 in Scorpius. Located about 400 light-years from Earth, it marks the central star of the Scorpion's head (or one of its claws). In 2000, Dschubba unexpectedly brightened by about half a magnitude and became a Be star, developing a gaseous disk — it had never shown this behavior before in recorded history.

Observing Tips

Dschubba sits at the head of Scorpius, forming a small line with Beta Sco (Graffias) and Pi Sco. It appears as a blue-white star. Its brightness has been variable since 2000, ranging between about 1.6 and 2.3, making it worth comparing with nearby stars of known brightness. Best observed June through August.

History

The name Dschubba comes from the Arabic 'al-jabha,' meaning 'the forehead.' Its unexpected transformation into a Be star in 2000 — after being stable for all of recorded history — was one of the most surprising stellar events observed in modern times.

Fun Facts

Dschubba's sudden transformation in 2000 from a normal B star to an emission-line Be star caught astronomers by surprise. A close periastron passage of its binary companion may have triggered mass transfer that created the gaseous disk. The star remains variable and unpredictable.

Observe

1Physical Properties

Magnitude 2.32
Range 1.6 - 2.3
Variable Type Gamma Cassiopeiae (Eruptive Be Star)
Spectral Type B0.3 IV subgiant
Star Color Blue (B-V -0.12)
Distance 396 ly

2Position & Identifiers

RA 16h 00m 20.0s
Dec -22° 37' 18.0"
Constellation Scorpius (Sco)
HR 5953
HIP 78401
HD 143275
SAO 184014
Bayer Delta
Flamsteed 7 Sco

3How easy to spot?

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Equipment Bortle 3 Bortle 4 Bortle 5
Naked eye Easy Easy Easy
50mm finder Easy Easy Easy
150mm scope 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 O
Separation 0.2″
Companion Mag 4.6
Companion Sp B2
Position Angle 16°
Star Colors A: Blue B: Blue
Discoverer LAB 3
Possible quadruple system: SB 3.0, 5.0v, sep. 0.00001", 3.3v at 0.1", and 4.9v at 0.186".

Separation over time

Period: 10.8 y Eccentricity: 0.939 Now: 0.18", PA 351° -0.06" in 5 years
0.00" 0.06" 0.11" 0.17" 0.22" 2022 2024 2026 2028 2030 0.18"

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

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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

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15Stellar Notes

Primary SB about 20d. Another companion 4.9v at 0.181", discovered by occultation and speckle interferometry, has | longer period. Resolved by speckle observations 1986.45, sep. 0.17".
Color excess E(B-V) = +0.16. Conspicuous infrared deficiency.
Sco OB2; Sco-Cen cluster; upper Sco region; HII region.
Dschubba; Iclarkrau.
Diam. = 0.00045 - 0.00046".
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Light Travel Time Machine

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Relativistic Travel

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