Chapter 22 Origin of Modern Astronomy

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Chapter 22

Origin of Modern Astronomy

Sec. 1 Early Astronomy

Astronomy—the science that studies the universe

• Properties of objects in space and the laws of the universe

• Greeks were the first to study the sun, moon, and stars

• Used geometry and trigonometry to measure sizes and distances

• Aristotle was the first to believe the Earth was round based on the curved shadow on the moon.

• His beliefs were abandoned in the Middle Ages.

The Geocentric Universe

• By the 2 nd Century B.C., the Greeks believed the Earth was a motionless sphere in the center of the universe.

Geocentric Model—(geo-Earth, centric-centered) the moon, sun, and known planets (Mercury, Venus, Mars, & Jupiter) orbit the Earth.

Orbit—the path of an object as it goes around another object in space

• Beyond the planets was a hollow sphere where the stars travelled daily around the Earth.

Early Astronomers

• Eratosthenes was the first to attempt to establish the size of Earth.

• By comparing the noontime sun and shadows in 2

Egyptian cities, and measuring the difference in angles between them, he was able to estimate the circumference of the Earth.

• Hipparchus was the first to create a star catalog.

• Divided almost 850 stars into 6 groups according to their brightness.

Ptolemaic System

• Claudius Ptolemy’s model of the universe (141 A.D) predicted the motion of the planets around the Earth.

• Each planet moves slightly eastward among the stars, but periodically each planet appears to stop, change direction for a while, then continue eastward again.

Retrograde Motion—the apparent westward drift of the planets.

• Ptolemy believed it resulted from planets moving along smaller circles, which then moved around the Earth.

• His theory predicted planetary motion well, and went unchallenged for 13 centuries.

Heliocentric Universe

• Ptolemy was WRONG! The planets do not orbit the Earth.

• Aristarchus was the first to propose a heliocentric universe.

• Helio-Sun Centric-Centered

• He used geometry to calculate distances and sizes of the sun and moon (although his calculations were too small)

Heliocentric Model—Earth and the other planets orbit the sun.

Modern Astronomy

• We now know that the universe is not heliocentric, but our solar system is.

Nicolaus Copernicus (2000 yrs after Aristarchus) proposed a model of the solar system with the sun at the center.

• It made more sense that Earth, rather than the sky, rotated once a day.

• He used perfect circles to represent the orbits of the planets, even though they strayed from his predicted position.

• This model also explained the retrograde motion of the planets

• The combination of the motion of Earth and the planet’s own motion around the sun.

• Different sized orbits make the planets appear to change speed and direction.

Tycho Brahe

• Danish, born 3 years after Copernicus died.

• Built instruments & angle-measuring devices which he used to measure the locations of the heavenly bodies (Before the telescope was invented)

• His observations, especially of Mars, were far more precise than earlier measurements.

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