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Alpha Arae — Star in Ara

Magnitude 2.8–2.9m Star Ara Visible
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About Alpha Ara

Description

Alpha Arae is a blue main-sequence star of spectral type B2Vne at magnitude 2.95, the brightest star in Ara (the Altar). Located about 270 light-years from Earth, it is a Be star — rapidly rotating and surrounded by a gaseous disk. Its luminosity is about 5,800 times solar.

Observing Tips

Alpha Ara lies in the southern part of the small constellation Ara, south of the Scorpion's tail. It is a blue-white star in a rich part of the southern Milky Way. Only visible from the southern hemisphere and very low northern latitudes. Best observed June through August.

History

Alpha Arae has no traditional proper name. Ara is one of the 48 Ptolemaic constellations, representing the altar on which the gods swore their oath before battling the Titans.

Fun Facts

Alpha Ara's Be-star disk was one of the first to be spatially resolved using optical interferometry, confirming that Be stars do indeed have equatorial disks of ejected gas as theorized.

Observe

1Physical Properties

Magnitude 2.95
Range 2.73 - 3.00
Period 23.6 hours
Variable Type Lambda Eridani (Be Star)
Spectral Type B2Ve
Star Color Blue (B-V -0.17)
Distance 266 ly

2Position & Identifiers

RA 17h 31m 50.5s
Dec -49° 52' 34.0"
Constellation Ara
HR 6510
HIP 85792
HD 158427
SAO 228069
Bayer Alpha

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 May – Jul (peak: Jun)

5Survey Image

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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

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15Stellar Notes

2.76 - 2.90V.
Companion K0IV, optical.
Cas-Tau group; member of the local association (Pleiades group); Sco-Cen assoc.; probable member of Sco-Cen cluster.
Shell star with variable H alpha emission.
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Light Travel Time Machine

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Relativistic Travel

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