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Black Genesis: The Prehistoric Origins of Ancient Egypt

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<strong>The</strong> surface <strong>of</strong> the now-covered bedrock was scoured by constant winds during many thousands <strong>of</strong> years <strong>of</strong> dry<br />

periods leading up to 9000 BCE. An area <strong>of</strong> s<strong>of</strong>ter bedrock was scoured more deeply by the winds, which created the<br />

depression that filled with water every summer season to become the playa during the monsoon season. This lasted to<br />

around 3500 BCE, after which the region became the hot, hyperdry place that it is today. <strong>The</strong> last humid period in the<br />

<strong>Egypt</strong>ian Sahara, which lasted from about 9000 BCE to 3500 BCE, seems also to have ended abruptly. Yet scientists<br />

also know that there have been several humid periods before this last one. Paleoclimatologists are finding that humid or<br />

wet periods in the Sahara occur with curious regularity, which suggests that these periods might be linked to Earth’s<br />

cyclical geological changes. Paleoceanographer and marine geologist Peter B. deMenocal studied sediment cores from<br />

the eastern Atlantic Ocean to measure the past climate <strong>of</strong> the Sahara. <strong>The</strong>se sediments, which were originally created by<br />

wind-carried dust and sand that then settled to the bottom <strong>of</strong> the ocean to form layers, act as graduations for measuring<br />

climate changes over long periods <strong>of</strong> time in the same way that rings in tree trunks can tell us <strong>of</strong> annual weather<br />

variations. <strong>The</strong> phases <strong>of</strong> the humid periods that deMenocal found in the ocean sediments matched those that the<br />

geologists found in the sediment layers at Nabta Playa. DeMenocal was able to show that the humid Sahara periods<br />

occurred regularly, about every twenty thousand years, and, furthermore, that they always began and ended suddenly.<br />

According to deMenocal, the cause <strong>of</strong> these sudden climate fluctuations from humid to dry were linked to the cyclical<br />

changes <strong>of</strong> Earth’s motion with respect to the fixed stars. 5<br />

<strong>The</strong> basis <strong>of</strong> deMenocal’s research relating climatic changes to the fixed stars began in 1920. Interestingly, in that<br />

same year Ahmed Hassanein and Rosita Forbes undertook their fateful expedition to the Kufra oasis (which eventually<br />

led to the discovery, a few years later, <strong>of</strong> the massifs <strong>of</strong> Jebel Uwainat and Gilf Kebir), and in that year the Serbian<br />

mathematician Milutin Milankovitch (1879–1958) published his controversial paper that would become a foundation in<br />

the science <strong>of</strong> climate change. 6 <strong>The</strong> Milankovitch Curve, as his theory is known, was based on an elegant and simple<br />

notion: the small, gradual, annual changes in Earth’s orbit around the sun as well as the spin <strong>of</strong> its axis when considered<br />

over many thousands <strong>of</strong> years will create sizeable recurring cycles causing Earth to receive sometimes more, sometimes<br />

less light and heat from the sun, which will cause significant climate changes. <strong>The</strong>se changes are the result <strong>of</strong> three<br />

phenomena <strong>of</strong> Earth’s movements: precession, obliquity, and eccentricity.<br />

1. Precession is a gyrating motion <strong>of</strong> Earth’s axis, which causes the planet to wobble like a spinning top, making a<br />

complete cycle every twenty-six thousand years or so.<br />

2. Obliquity is the angle <strong>of</strong> tilt that Earth’s axis makes with the plane <strong>of</strong> its orbit around the sun. This angle moves up<br />

and down in a slow cycle <strong>of</strong> about forty-one thousand years, known as the obliquity <strong>of</strong> the ecliptic. Today the angle<br />

is 23.4 degrees, but, for example, in 5000 BCE it was about 24.1 degrees. Like the precession cycle, astrophysicists<br />

today can calculate with a great deal <strong>of</strong> accuracy exact changes in past and future obliquity. 7<br />

3. Eccentricity is the elongatedness (that is, the perihelion and aphelion) <strong>of</strong> Earth’s elliptical orbit around the sun,<br />

which changes in a complex cycle <strong>of</strong> about one hundred thousand years. *4<br />

Precession and the Zodiacal Belt<br />

<strong>The</strong> sun at the equinoxes (March 21 and September 22) is located in the sky against a backdrop <strong>of</strong> a particular group <strong>of</strong><br />

stars or constellations that lie along the so-called zodiacal belt. Every year the position <strong>of</strong> the sun along the zodiacal belt<br />

at the equinoxes moves, or precesses, a tiny amount so that, in about twenty-six thousand years, the sun makes a<br />

complete cycle around the entire zodiac. Although the precise number <strong>of</strong> years per each full precession cycle always<br />

changes a bit, astrophysicists today can calculate the duration <strong>of</strong> precessional cycles, past and future, with a great deal<br />

<strong>of</strong> accuracy. 8<br />

<strong>The</strong>se three effects—precession, obliquity, and eccentricity—when taken together, cause long-term climate change<br />

every twenty thousand to twenty-six thousand years—such as, for example, the great ice ages known to have occurred in

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