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Achernar

HIP 7588; Alpha Eri

HIP 7588; Alpha Eri DoubleStar Eri Visible Level 5 Expert level - Requires steady seeing
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Physical Properties

Magnitude 0.46
Variable Type Eclipsing Binary (Beta Lyrae-type)
Spectral Type B6Vep
Star Color Blue (B-V -0.16)
Temperature 14988 K
Radius 9.3 R☉
Distance 144.0 ly

Position & Identifiers

RA 01h 37m 42.9s
Dec -57° 14' 12.0"
Constellation Eri
HR 472
HIP 7588
Bayer Alpha
Variable ID Var

Visibility

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Multiple Star System

Separation 0.3″
Companion Mag 2.1
Companion Sp A2V
Position Angle 309°
Star Colors A: Blue B: White
Discoverer KRV 54

Eyepiece View

80x Dawes: 1.9″ TFOV: 0.6°
Realistic = true angular size
N E 309° A (0.5) B (2.1)

Sep: 0.3″ · PA: 309° · N up, E left

Unresolved · Rayleigh: 2.3″ · Dawes: 1.9″ · Eff: 3.1″

Size Comparison

Stellar Lifecycle

Spectral Classification

Hertzsprung-Russell Diagram

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Blackbody Spectrum

Stellar Absorption Spectrum

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

Stellar Notes

EB or Ell, amp. 0.02V. H alpha var. emission and possible high-velocity mass loss. Expanding circumstellar shell.
Member of Pleiades group.
Lyman alpha and Lyman beta observed from COPERNICUS. H alpha and H beta var. emission and possible high-velocity mass | loss. Expanding circumstellar shell.
Period in RV and light (1.26d) seems best explained by rotation. Weak but significant variations in strength of | MgII 4481. RV of H gamma and HeI 4471 consistent with period, amp. 30k/s. Variable light amp. 0.02V.
ACHERNAR.
Diam. = 0.00185 - 0.00192".

Survey Image

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About Achernar

Description

Achernar is the brightest star in the constellation Eridanus and the ninth brightest in the night sky at magnitude 0.46. It is a blue main-sequence star of spectral type B6V, located about 139 light-years from Earth. Achernar is roughly 6-7 times the mass of the Sun and about 3,000 times more luminous. It is one of the flattest stars known, spinning so rapidly (at about 250 km/s at its equator) that its equatorial diameter is about 56% larger than its polar diameter.

Observing Tips

Achernar marks the southern end of the long, winding constellation Eridanus (the River). It is visible only from latitudes south of about 33°N. Its brilliant blue-white color and isolated position make it easy to identify from the Southern Hemisphere. There are few other bright stars in its immediate vicinity, which makes it stand out dramatically. Best observed from October through January from southern latitudes.

History

The name Achernar derives from the Arabic 'Akhir an-Nahr' meaning 'the end of the river,' referring to its position at the southern terminus of Eridanus. Because of its far southern declination (-57°), it was unknown to ancient Greek and Roman astronomers, who instead placed the end of their river constellation at the star Acamar (Theta Eridani). Achernar was added to European star catalogs after the great southern voyages of exploration.

Fun Facts

Achernar's extreme oblateness was directly measured by ESO's VLTI interferometer in 2003, confirming that it is the flattest star ever directly observed. If the Sun rotated as fast as Achernar, a day would last only about 5 hours. Achernar also has a close companion star (spectral type A) that orbits with a period of about 15 years.