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History of Astronomy The knowledge of the Ancients

History of Astronomy

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History of Astronomy. The knowledge of the Ancients. Passage of astronomical knowledge. Ancient Babylon. Ancient Egypt. Ancient Greece. Ancient Roman Empire. Mesopotamia/Babylon. Modern political boundaries. Ancient Babylon. Mesopotamia/Babylon. Ancient Egypt. Nile River Valley. - PowerPoint PPT Presentation

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Page 1: History of Astronomy

History of Astronomy

The knowledge of the Ancients

Page 2: History of Astronomy

Passage of astronomical knowledgeAncientBabylon

AncientEgypt

AncientGreeceAncient Roman Empire

Page 3: History of Astronomy

Mesopotamia/BabylonModern political boundaries

Ancient Babylon

Page 4: History of Astronomy

Mesopotamia/Babylon

Page 5: History of Astronomy

Ancient Egypt

Nile River Valley

Great Pyramid ofKufu

Page 6: History of Astronomy

Ancient Greece

Page 7: History of Astronomy

What did ancient civilizations achieve in astronomy?

• Daily timekeeping • Tracking the seasons and calendar• Monitoring lunar cycles• Monitoring planets and stars• Predicting eclipses• And more…

Page 8: History of Astronomy

Ancient people of central Africa (6500 B.C.) could predict seasons from the orientation of the crescent moon.

Page 9: History of Astronomy

• Egyptian obelisk: Shadows tell time of day.

Page 10: History of Astronomy

England: Stonehenge (completed around 1550 B.C.)

Page 11: History of Astronomy

Scotland: 4,000-year-old stone circle; Moon rises as shown here every 18.6 years.

Page 12: History of Astronomy

Mesopotamian Astronomy

• MESOPOTAMIANS built observatories starting ~6000 years ago:

• the ziggurats had seven levels, one for each wandering object in the sky:

• Sun, Moon, Mercury, Venus, Mars, Jupiter, Saturn• Thus 7 days to the week• They tracked stars --- groups rising before sun at

different times of year implied seasonal beginnings for planting and

harvesting (zodiac).• Divided circles in 360 degrees,

each degree into 60 minutes and each minute into 60 seconds -- we still use!

• Left written records in cuneform so we understand them better

Page 13: History of Astronomy

Other Ancient Accomplishments

• Mesopotamians could predict planetary positions -- synodic periods, e.g., Mars returns to same location roughly every 780 days:

22 synodic periods = 47 years, so• records of old planetary positions could give good

locations.• Knew about the SAROS cycle 2700 years ago: lunar

eclipses definitely occurred every 18.6 years.• Chinese, Indians and Mayans also knew these

patterns• Egyptians used astronomical events to forecast Nile

floods and harvest times.

Page 14: History of Astronomy

Mesopotamian Astronomy and Influence

• By 2000 BC Ur and other Sumerian and Babylonia cities had large temples, or ziggurats, usually aligned N-S, like most Egyptian pyramids

• Egyptian and Mesopotamian knowledge spread to Europe, Asia and Africa

Page 15: History of Astronomy

Cuneiform- first system of writing

Page 16: History of Astronomy

Cuneiform tablet with envelope

Page 17: History of Astronomy

Greek Astronomy

Page 18: History of Astronomy

Greek Astronomy• About 624 BC to 547 BC• One of the earliest

Greek philosophers.• His areas of interest

included geometry and astronomy.

• There are no books or writings that have survived from Thales.

Page 19: History of Astronomy

Greek Astronomy• About 569 BC to 475 BC• One of the greatest

mathematicians of all time.• Founded secret society

based on his mathematical discoveries and their religious implications.

• Since the society was extremely secretive, very little is known about his life or personal works.

Page 20: History of Astronomy

Greek Astronomy• 427 BC to 347 BC• Well known for political and

social philosophy but he also made contributions to astronomy.

• He was most noted for his belief in the perfect and unchanging nature of the heavens.

• Plato was the head of the School of Athens & was Aristotle’s teacher.

Page 21: History of Astronomy

Greek Astronomy• 384 BC to 322 BC• Founded his own school

called the Lyceum in Athens• Made contributions to all

areas of philosophy but math was his weakness

• He did not believe that empirical evidence was necessary to prove ideas.

Page 22: History of Astronomy

Greek Astronomy• Aristotle is one the first to

attempt to create a scientific model of the universe.

• This model has now become known as the “Geocentric Model” which places the “imperfect” Earth at the center and all of the “perfect” celestial objects go around us in perfect circular motion

Page 23: History of Astronomy

Greek Astronomy

• About 325 BC to 265 BC• Great mathematician but so

little is known about him that people question whether he was an actual person or a group of mathematicians.

Page 24: History of Astronomy

Greek Astronomy• The book “Elements” is

possible the most famous and long lasting math text books in history.

Page 25: History of Astronomy

Greek Astronomy

• About 310 BC to 230 BC• We have no writings that

have survived but Aristarchus is referred to in the writings of other philosophers

Page 26: History of Astronomy

Greek Astronomy

• Most noted for proposing the idea of a heliocentric universe with the earth as one of the planets moving around the Sun.

• Aristarchus is the first to attempt to measure the relative distance between the Earth-Moon and the Earth-Sun without the aid of trigonometry.

• Actual angle = 89° 50” not 87°

Page 27: History of Astronomy

Greek Astronomy

• 276 BC to 194 BC• Librarian at the Great Library of

Alexandria in Egypt.• Developed a calendar with a

leap year.• Measured the circumference of

the Earth in 325 BC !!• Achieved an accuracy of about

90% of the actual number.

Page 28: History of Astronomy

Eratosthenes measures the Earth (c. 240 B.C.)

Measurements:Syene to Alexandria • distance ≈ 5,000 stadia• angle = 7°

Page 29: History of Astronomy

Eratosthenes measures the Earth (c. 240 B.C.)

Calculate circumference of Earth:7/360 (circum. Earth) = 5,000 stadia circum. Earth = 5,000 360/7 stadia ≈ 250,000 stadia

Compare to modern value (≈ 40,100 km): Greek stadium ≈ 1/6 km 250,000 stadia ≈ 42,000 km

Page 30: History of Astronomy

Greek Astronomy• 190 BC to 120 BC• Hipparchus is consider the first great astronomer

and scientist• Hipparchus is one of the first of the ancient

philosophers to realize that ideas must be proven with empirical evidence.

• He realized that more data meant more certainty in the idea or model

Page 31: History of Astronomy

Greek Astronomy

• Created highly accurate star atlases in an attempt to measure the length of the year more accurately.

• He measured the length of the year to within 6.5 minutes of the actual time.

• He discovered precession by examining ancient star position data (mostly Mesopotamian) and comparing them to his own measurements.

Page 32: History of Astronomy

Greek Astronomy

• Based on measurements during an eclipse, he is able to place a range on the distance to the moon.

• He estimated it to be between 59 and 67 Earth diameters. The actual number is 60.

• He marks the first truly scientific astronomical mind and his influence is still felt today.

Page 33: History of Astronomy

Greek Astronomy• About 85 AD to 165 AD• Ptolemy is the most influential

astronomer in his day and his models of the universe will prevail for the next 1400 years

• He is a great admirer of Hipparchus and his rigorous method of verifying ideas with empirical data.

• Ptolemy is also accused of stealing ideas without crediting his source.

Page 34: History of Astronomy

Greek Astronomy• Ptolemy is a great proponent of the

geocentric model.• He saw that there were problems

with Aristotle’s simplistic idea of a geocentric model.

• Ptolemy employed an old idea of epicycles to explain help explain the discrepancies in the evidence for geocentrism.

• Although he was able to make more accurate predictions than previous astronomers, his model still failed to be completely accurate.

Page 35: History of Astronomy

• Greeks were the first people known to make models of nature.

• They tried to explain patterns in nature without resorting to myth or the supernatural.

Greek geocentric model (c. 400 B.C.)

Why does modern science trace its roots to the Greeks?

Page 36: History of Astronomy

Two Different Early Models…

• GEOCENTRIC– Earth is the center of everything– Earth doesn’t spin or move

Page 37: History of Astronomy

Two Different Early Models…

• HELIOCENTRIC

– The Sun is the center of the solar system

– Earth spins (rotates) to create day/night

– Earth orbits (revolves)to create the year

Page 38: History of Astronomy

Geocentric Models made “sense”

• GEOCENTRIC: Earth doesn’t move– If we did, we’d feel it!– If we did, we’d lose the moon!– If we did, the stars around us would shift!

• THEREFORE:– Sky (& Stars!) rotated around us

– Sun & Moon & Planets actually move among key constellations of the Zodiac by design/choice

Page 39: History of Astronomy

Two Different Early Models…• HELIOCENTRIC: Earth moves about the Sun

– So do all of the planets– The Moon goes around us, too– Earth spins to create night and day

• THEREFORE:– Sky (& Stars!) just SEEM to rotate around us

– Sun & Moon & Planets moved among key constellations of the Zodiac because of OUR motion

Page 40: History of Astronomy

Parallax

Page 41: History of Astronomy

• Parallax results from shift in viewing position

• If CLOSE to Earth, a star would be seen in different locations (at different angles)

Page 42: History of Astronomy

• Parallax results from shift in viewing position

• If FAR from Earth, a star would NOT be seen in different locations (at different angles)

Page 43: History of Astronomy

KEY IDEA: Retrograde motion of the planets

• We make the observation that planets – and only the planets – “dance” in front of the stars. How is this observation explained in each model?

Page 44: History of Astronomy

The Motion of the Planets

in the sky over time

Page 45: History of Astronomy

The Motion of Mars

In 2009-2010

Page 46: History of Astronomy

Retrograde Motion Explanations

• Ancient (and geocentric)– The planets move on their own around us– God(s) control their motions– Heaven’s realm – doesn’t concern us!– It just is…

Page 47: History of Astronomy

Ptolemaic Retrograde Motion

Page 48: History of Astronomy

So how does the Ptolemaic model

explain retrograde motion?

Planets really do go backward in this

model.

Page 49: History of Astronomy

Retrograde Motion Explanations

• Modern (and heliocentric)

– Earth and other planets orbit the sun at different rates

– Earth “laps” slower-moving outer planets – and they appear to loop

Page 50: History of Astronomy
Page 51: History of Astronomy

Geocentric or Heliocentric?

• Of the early philosophers, only Hipparchus favored the heliocentric model

• Most philosophers thought that the evidence supported the Geo model more than the Helio model

• What was the evidence? Let’s Look….

Page 52: History of Astronomy

Geocentric Evidence Everything appears to revolve

around the Earth each day (diurnal motion).

There is no observable parallax of the stars, planets, Moon, or Sun.

The motions of the stars and heavens are perfect circles.

The heavens were unchanging but the Earth was not.

Page 53: History of Astronomy

Problems With the Geocentric Model The planets appear to change brightness,

implying a change of distance. The planets undergo retrograde motion (they

move backwards compared to the direction the Sun moves).

The Sun, Moon, and Planets do not move at the same speed all the time.

Mercury and Venus are never seen at opposition (they always appear close to the Sun.

Page 54: History of Astronomy

Evidence of the Heliocentric Model The changing brightness of the planets is

explained by the Earth getting closer and farther from the planets during our orbit of the Sun.

Our passing planets explain the retrograde motion of the outer planets.

Mercury and Venus are not seen at opposition because they orbit the sun, just as we do.

Page 55: History of Astronomy

Problems with the Heliocentric Model The changing speeds of the Sun, Moon, and

planets is not explained by simply placing the Sun at the center of the universe.

We do not feel the Earth moving or the atmosphere being pulled away as we fly around the Sun.

If the Earth were spinning, wouldn’t we be thrown off into space?

Why is there no parallax due to our spin or our orbit?

Page 56: History of Astronomy

So Which is Right? The ancients favored the

geocentric model because it seemed impossible to believe that the Earth was moving.

During ancients times, the mathematical and scientific tools were not available to answer the question without dispute.