un:almagest-revolutions
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===== - Enuma Anu Enlil ===== | ===== - Enuma Anu Enlil ===== | ||
- | To begin the story of the *Almagest*, we have to start with another book: the astrology text *Enuma Anu Enlil* (meaning | + | To begin the story of the 'Almagest', we have to start with another book: the astrology text 'Enuma Anu Enlil' |
- | It was because the authors of *Enuma* closely observed the motions of the Moon, the Sun, and the five visible planets relative to the fixed stars over at least seven centuries that the first cosmological model could be developed—the | + | It was because the authors of 'Enuma' |
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The practice of creating ephemerides—tables listing the past and future positions of the Moon, Sun, and planets—began in Babylon. For this, they not only measured angular positions but also began calculating velocities. For example, above is a graph showing the change in the **Sun’s angular velocity** over a year, based on data from a Babylonian tablet dated to 132 BCE. Relative to the background of “fixed” stars, the Sun moves 360 degrees in a year. The graph shows how much distance it covers each month as velocity. We see that in the second month, the Sun's angular velocity decreases to a minimum (around 28 degrees/ | The practice of creating ephemerides—tables listing the past and future positions of the Moon, Sun, and planets—began in Babylon. For this, they not only measured angular positions but also began calculating velocities. For example, above is a graph showing the change in the **Sun’s angular velocity** over a year, based on data from a Babylonian tablet dated to 132 BCE. Relative to the background of “fixed” stars, the Sun moves 360 degrees in a year. The graph shows how much distance it covers each month as velocity. We see that in the second month, the Sun's angular velocity decreases to a minimum (around 28 degrees/ | ||
- | They had two methods to explain exactly how the velocity changed. In one method, it was assumed that the Sun's velocity remained constant for half the year, then shifted once, remaining constant again for the other half. In the other method, it was proposed that the Sun’s velocity steadily increased over half the year and steadily decreased over the other half. Humans first applied calculations of displacement, | + | They had two methods to explain exactly how the velocity changed. In one method, it was assumed that the Sun's velocity remained constant for half the year, then shifted once, remaining constant again for the other half. In the other method, it was proposed that the Sun’s velocity steadily increased over half the year and steadily decreased over the other half. Humans first applied calculations of displacement, |
===== - From Arithmetic to Geometry ===== | ===== - From Arithmetic to Geometry ===== | ||
- | Babylonian astronomers emphasized arithmetic, while the Greeks emphasized geometry. Since the moon, sun, and planets actually follow geometric paths, Greek predictions were easier | + | Babylonian astronomers emphasized arithmetic, while the Greeks emphasized geometry. Since the moon, sun, and planets actually follow geometric paths, Greek predictions were easier. Analyzing all the data, the Greeks created a geocentric model of the universe. The first major contribution to this model was made by the Greek philosopher Anaximander from the city of Miletus in Turkey. According to him, the Earth is a cylinder fixed at the center of the universe, with humans living on one flat surface; everything in the sky revolves around it; the sun is the farthest, followed by the moon, then all the stars, and the five planets closest to the Earth. |
Pythagoras' | Pythagoras' | ||
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In the work of transforming astronomy from mathematics to physics through cosmology, Galileo' | In the work of transforming astronomy from mathematics to physics through cosmology, Galileo' | ||
- | By the time Newton published | + | By the time Newton published |
===== - Proof of Revolutions ===== | ===== - Proof of Revolutions ===== | ||
+ | ==== - Aberration: 1720s ==== | ||
To understand the first observational proof of the ' | To understand the first observational proof of the ' | ||
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One of the greatest astronomers of the eighteenth century, England' | One of the greatest astronomers of the eighteenth century, England' | ||
+ | ==== - Parallax: 1830s ==== | ||
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