How the Greeks Knew Earth is Spherical PDF

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ancient greek science spherical earth historical science scientific method

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This lesson explores how ancient Greek thinkers determined the Earth's shape. Using observations of stars, lunar eclipses, and ships disappearing over the horizon, they developed the idea of a spherical Earth, influencing future scientific inquiry and navigation.

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How the Greeks Knew the Earth is Spherical Agenda Introduction Geometric and Mathematical Proofs Early Greek Observations Impact on Navigation Aristotle's Contributions Eratosthenes' Experiment...

How the Greeks Knew the Earth is Spherical Agenda Introduction Geometric and Mathematical Proofs Early Greek Observations Impact on Navigation Aristotle's Contributions Eratosthenes' Experiment Testimonies from Historical Texts Lunar Eclipses Scientific Legacy Observations of Stars Key Metrics and Figures Ships Disappearing Over the Horizon Summary Philosophical Arguments Conclusion Introduction Introduction Understanding how the ancient Greeks came to the conclusion that the Earth is spherical is crucial for appreciating the development of scientific thought. This knowledge highlights the Greeks' use of observation, reasoning, and experimentation, laying the foundation for modern science. It also demonstrates the importance of questioning established beliefs and seeking evidence-based conclusions. By exploring the methods and evidence used by the Greeks, we gain insight into the origins of scientific inquiry and the progress of human understanding of the natural world. Early Greek Observations Observations Early Greek philosophers, such as Pythagoras and Parmenides, began to question the flat Earth model. Pythagoras, in the 6th century BCE, observed that the Moon and other celestial bodies were spherical, leading him to propose that the Earth might also be a sphere. Parmenides, in the 5th century BCE, suggested a spherical Earth based on the reasoning that a sphere is the most harmonious and perfect shape. These early observations and philosophical reflections laid the groundwork for later, more empirical investigations into the Earth's shape. Evidence Aristotle's Contributions Lunar Eclipses Visibility of Stars Shape of Earth's Shadow Aristotle noted that Earth's He observed that travelers going He argued that the consistent shadow on the moon during a south saw southern round shape of Earth's shadow lunar eclipse is always round, constellations rise higher above on the moon during different which can only be explained if the horizon, indicating a curved lunar eclipses supports the idea Earth is spherical. surface. of a spherical Earth. Methodology Eratosthenes' Experiment Conceptualization Measurement Calculation Result Analysis Eratosthenes hypothesized that On the summer solstice, Eratosthenes used the Eratosthenes concluded that by measuring the angle of the Eratosthenes measured the angle difference in angles and the the Earth's circumference was sun's rays at two different of the sun's rays in Alexandria, known distance between approximately 40,000 where it cast a shadow, and noted locations, he could calculate Alexandria and Syene to kilometers, remarkably close to that in Syene, the sun was directly the Earth's circumference. overhead. calculate the Earth's modern measurements. circumference. Hypothesis formulation Angle of shadow in Distance between Alexandria Calculated Earth's Identification of Alexandria: ~7.2 degrees and Syene: ~800 km circumference: ~40,000 km measurement locations: No shadow in Syene Calculation formula: (360 Comparison with modern degrees / angle difference) x Alexandria and Syene value: ~40,075 km distance between locations Observations Lunar Eclipses During a lunar eclipse, the Earth comes between the Sun and the Moon, casting a shadow on the Moon's surface. Ancient Greek astronomers observed that this shadow was always round, regardless of the Earth's orientation. This consistent round shape could only be produced by a spherical object, as a flat or differently shaped Earth would cast elongated, distorted shadows. These observations provided compelling evidence to the Greeks that the Earth was not flat, but instead a sphere. Evidence Observations of Stars Changing Constellations As one travels north, certain southern constellations disappear below the horizon Conversely, traveling south reveals new constellations not visible from northern regions The gradual shift in visible stars indicates a curved surface, supporting a spherical Earth Latitude and Star Visibility The altitude of the North Star (Polaris) changes with latitude, appearing higher in the sky as one moves north At the equator, Polaris lies on the horizon, while it becomes invisible from the southern hemisphere Plus tip: To customize, add specific examples Consistent changes in star positions with latitude provide strong evidence for Earth's of constellations or historical sphericity anecdotes about Greek travelers and their star observations. Evidence Ships Disappearing Over the Horizon One of the compelling pieces of evidence for a spherical Earth observed by the Greeks was the phenomenon of ships disappearing hull-first over the horizon. As a ship sails away from shore, it seems to sink gradually, with the hull vanishing first, followed by the mast and sails. This occurs because the Earth's surface is curved. If the Earth were flat, the entire ship would simply appear smaller and smaller, but remain visible in its entirety. This observation was crucial in supporting the idea that the Earth is not flat, but rather a sphere. Arguments Philosophical Arguments Sphere as a Perfect Shape Plato and Pythagoras viewed spheres as perfect, harmonious shapes. A sphere has no edges, making it symbolically fitting for the Earth. Perfect symmetry of a sphere was seen as a reflection of celestial perfection. Symmetry and Balance A spherical Earth ensured balance and stability in the cosmos. Greeks believed that the universe's symmetry necessitated a spherical Earth. Philosophers argued that natural forms, like planets, are spherical due to Plus tip: gravity. Customize this slide with additional philosophical perspectives or historical context relevant to your audience. and Euclid, provided geometric and Proofs mathematical proofs supporting a spherical Earth. Pythagoras, around 500 BCE, proposed that the Earth was spherical based on the idea that a sphere was the perfect Geometric and shape. Euclid’s geometry laid the Mathematical Proofs groundwork for understanding celestial mechanics. Later, Archimedes used geometric principles to explain the curvature Plus tip: Customize this slide by adding of the Earth. These proofs demonstrated that diagrams or illustrations of geometric proofs from ancient Greek texts to visually support the explanations. the properties of a sphere, such as the way Navigation Impact on Navigation Enhanced Route Planning Expansion of Trade Understanding Earth's curvature Enabled longer voyages with allowed more accurate sea better accuracy. routes. Facilitated trade routes extending Greeks could anticipate the beyond the Mediterranean. horizon and navigate accordingly. Increased safety and Helped in creating more precise predictability in maritime travel. maps and charts for navigation. Plus tip: Add specific examples of Greek voyages that benefited from the understanding of a spherical Earth, such as journeys to distant colonies or trade expeditions. Evidence "The Earth is spherical, and the differences in the stars seen in different Testimonies from places are a proof of this. The shape of its Historical Texts shadow, which is always circular and not stretched out, as it would be if it were flat, is another proof." Aristotle, 'On the Heavens' Legacy Scientific Legacy Foundation for Astronomy Advances in Navigation Influence on Scientific Method Greek discoveries about Earth's Understanding Earth's sphericity Greek emphasis on observation shape laid the groundwork for enabled more accurate and reasoning set a precedent future astronomical studies, navigation and cartography, for the scientific method, influencing figures like Ptolemy benefiting explorers like impacting disciplines beyond and Copernicus. Christopher Columbus and astronomy and geography. Ferdinand Magellan. Discoveries Key Metrics and Figures 40,075 39,375 km km Earth's Eratosthenes' Circumference Estimate 800 km 7.2° Alexandria-Syene Sun's Angle Distance Difference Plus tip: You can customize the metrics with more detailed data or additional figures from other Greek scientists to enrich the slide. Conclusion Summary Early Greek philosophers began to question the flat Earth model through various observations. Aristotle provided strong arguments for a spherical Earth by observing lunar eclipses and star visibility. Eratosthenes accurately measured the Earth's circumference using the angles of the sun's rays in different locations. The shape of the Earth's shadow during lunar eclipses and the phenomenon of ships disappearing hull-first over the horizon supported the spherical Earth theory. Greek understanding of a spherical Earth influenced navigation and exploration, leaving a lasting scientific legacy. Conclusion Greek discoveries about Earth's shape laid the foundation for modern astronomy and geography. Greek philosophers and scientists, through observations, logical reasoning, and mathematical calculations, provided compelling evidence that the Earth is spherical. These discoveries were crucial in advancing navigation and exploration and set the stage for future scientific endeavors. The methodologies developed by the Greeks, such as Eratosthenes' measurement of Earth's circumference, are still appreciated for their ingenuity and accuracy. Thank you

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