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Achernar — Double Star in Eridanus

HIP 7588; Alpha Eridani

Magnitude 0.4–0.5m DoubleStar Eridanus (Eri) Visible
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About Achernar

Description

Achernar is the ninth brightest star in the sky at magnitude 0.46, a hot blue main-sequence star of spectral type B3Vpe in Eridanus. Located about 139 light-years from Earth, it has a luminosity of roughly 3,150 times solar. Achernar is the flattest star known — it spins so rapidly (at about 250 km/s) that its equatorial diameter is more than 50% larger than its polar diameter.

Observing Tips

Achernar marks the southern end of the long, winding constellation Eridanus (the River). It is a brilliant blue-white star visible from latitudes south of about 33°N. From the southern hemisphere it is prominent in the evening sky during southern spring and summer. It lies roughly between the south celestial pole and Canopus. Best observed October through January.

History

The name Achernar comes from the Arabic 'akhir al-nahr,' meaning 'the end of the river,' referring to its position at the terminus of Eridanus. The ancient Greeks could see a different star at Eridanus's end — Theta Eridani (Acamar) — because precession has shifted the sky since their time, bringing Achernar higher for classical observers' latitudes.

Fun Facts

Achernar's extreme oblateness makes it one of the most distorted stars known — if you could see it up close, it would look like a squashed ball rather than a sphere. Interferometric measurements confirmed this remarkable shape in 2003. It is the brightest and hottest star in the sky to be classified as a main-sequence Be star.

Observe

1Physical Properties

Magnitude 0.46
Range 0.44 - 0.54
Period 30.3 hours
Variable Type BE
Spectral Type B6Vep
Star Color Blue-white (B-V -0.16)
Temperature 14988 K
Radius 9.3 R☉
Distance 144 ly

2Position & Identifiers

RA 01h 37m 42.9s
Dec -57° 14' 12.0"
Constellation Eridanus (Eri)
HR 472
HIP 7588
HD 10144
SAO 232481
Bayer Alpha
Variable ID Var

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 Sep – Nov (peak: Oct)

5Light Curve

6Multiple Star System

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

Separation over time

Period: 7.0 y Eccentricity: 0.726 Now: 0.30", PA 304° -0.08" in 5 years
0.00" 0.09" 0.17" 0.26" 0.34" 2023 2024 2025 2026 2027 2028 2029 0.30"

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

Explore

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Size Comparison

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Compare Stars

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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

16Stellar 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".
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Light Travel Time Machine

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Relativistic Travel

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