How humanity moved from a static Earth to a universe of countless distant galaxies.

How Astronomy Changed our View of the Cosmos: from Gresham to the 21st Century · 54:52 · Video: Gresham College · Watch at the source

In short: For centuries, we believed the Earth sat motionless at the center of a starry sphere. Today, we know our galaxy is just one of many in an expanding cosmos. This transformation was driven by centuries of evolving technology, from simple naked-eye measurements to the precision of modern space-based telescopes.

Early astronomy was a practical necessity, used by ancient civilizations to track time for agriculture, navigation, and religious rituals. By 1000 BCE, Assyro-Babylonian astronomers were already recording periodic celestial motions. In the third century BCE, Greek thinkers like Aristarchus of Samos proposed a heliocentric system, though the geocentric model remained dominant. Hipparchus of Nicaea later compiled the first stellar catalogue in the second century BCE, using instruments like armillary spheres to map 850 stars with naked-eye precision. This tradition of observation was preserved and refined by Islamic scholars, such as Ulugh Beg, who built massive instruments like a 36-meter sextant in the fifteenth century.

The Renaissance brought a paradigm shift when Nicolaus Copernicus published his heliocentric theory in 1543, challenging the long-held belief that Earth was the center of the universe. However, the most radical changes followed the invention of the telescope in 1608. Galileo’s subsequent use of the instrument in 1609 shattered the notion of solid, transparent heavenly spheres. Later, Tycho Brahe’s observations of a comet moving freely through the planetary realm further dismantled ancient cosmic models. By the late 1800s, the integration of photography allowed astronomers to record faint objects that were previously invisible, moving beyond subjective hand-drawn sketches to objective, detailed data.

The 20th century solidified our modern understanding of the universe's scale. Using the 100-inch telescope at Mount Wilson Observatory, Edwin Hubble demonstrated in 1924 that the Milky Way is merely one of countless galaxies. This discovery expanded the known universe from a localized sky of stars to a vast, expanding realm. Today, astronomers continue to build upon these foundations, utilizing increasingly sophisticated technology to probe cosmic origins and the existence of planets around distant stars, proving that our view of the cosmos remains a work in progress.

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