Achernar — Double Star in Eridanus
HIP 7588; Alpha Eridani
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
2Position & Identifiers
3How easy to spot?
| Equipment | Bortle 3 | Bortle 4 | Bortle 5 |
|---|---|---|---|
| Naked eye Naked eye | Easy | Easy | Easy |
| 50 mm finder 50mm finder | Easy | Easy | Easy |
| 150 mm telescope 150mm scope | Easy | Easy | Easy |
Bortle 3 = rural · 4 = outer suburbs · 5 = suburbs
4Visibility
Set a location in User Settings to see visibility data.
5Light Curve
6Multiple Star System
Separation over time
Apparent separation over time, computed from ORB6 orbital elements. Steep curves indicate fast-changing pairs — catch them while they're splittable.
Explore
8
Size Comparison
9
Compare Stars
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Spectral Classification
11
Hertzsprung-Russell Diagram
12
Stellar Lifecycle
13
Blackbody Spectrum
14
Stellar Absorption Spectrum
Simulated absorption spectrum based on spectral type. Hover over lines to identify elements.
15
Stellar Fusion
Discover
16Stellar Notes
17
Light Travel Time Machine
18
Relativistic Travel
Nearby in the Sky
Other targets within a few degrees — pan your scope a little and keep exploring.
Visibility scores assume a 150 mm Newton at Bortle 4.
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