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Sharatan — Star in Aries

HIP 8903; Beta Arietis; 6 Arietis

Star Aries (Ari) Visible
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About Sharatan

Description

Sheratan is a white star of spectral type A5V at magnitude 2.64, the second brightest star in Aries. Located about 60 light-years from Earth, it has a luminosity of about 11 times solar. Sheratan is a spectroscopic binary with an orbital period of about 107 days.

Observing Tips

Sheratan lies just southwest of Hamal (Alpha Ari), forming the most visible pair of stars in the Ram's head. Together with Mesarthim (Gamma Ari), they define the small triangular head of Aries. Best observed October through February.

History

The name Sheratan comes from the Arabic 'al-sharatan,' meaning 'the two signs,' referring to Sheratan and Mesarthim as markers of the vernal equinox around 2000 BC. The precession of the equinoxes has long since moved the vernal point westward into Pisces.

Fun Facts

Sheratan marked the vernal equinox around the time of the early Babylonian astronomers, making it and its neighbor one of the most symbolically important pairs of stars in ancient astronomy.

Observe

1Physical Properties

Magnitude 2.64
Variable Type Delta Scuti (Pulsating)
Spectral Type A5. V SB
Star Color White (B-V 0.13)
Distance 59 ly

2Position & Identifiers

RA 01h 54m 38.4s
Dec +20° 48' 29.0"
Constellation Aries (Ari)
HR 553
HIP 8903
HD 11636
Bayer Beta
Flamsteed 6 Ari

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)

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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

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Stellar Fusion

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14Stellar Notes

Delta Sct?
106.9973d, K 37.1k/s, V0 -4.0k/s, asini 23.8. One of the most eccentric orbits known: e 0.892. Binary unresolved by | speckle interferometry 1981.69. SB2 in infrared: near-IR reticon spectra at 8800 Ang show double lines and indicate | that the secondary is late F- or G-type main-sequence star.
Sharatan; Sheratan; Al Sharatain.
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Light Travel Time Machine

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Relativistic Travel

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