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
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.
Explore
6
Size Comparison
7
Compare Stars
8
Spectral Classification
9
Hertzsprung-Russell Diagram
10
Stellar Lifecycle
11
Blackbody Spectrum
12
Stellar Absorption Spectrum
Simulated absorption spectrum based on spectral type. Hover over lines to identify elements.
13
Stellar Fusion
Discover
14Stellar Notes
15
Light Travel Time Machine
16
Relativistic Travel
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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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