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HISTORY OF ASTRONOMY
Early Astronomy


Astronomy is the science
studying outer space and the
universe.
 The

“Golden Age” of astronomy
was centered in Greece.
Early Astronomy


The Greeks took measurements
of distant objects such as the
Sun and the moon.



Famous Greek
philosopher, Aristotle, conclude
d Earth is round because it
always cast a curved shadow on
the moon.



Another Greek
astronomer, Hipparchus, deter
mined the location of almost

Aristotle (384-322 B.C.)

Hipparchus (190-120
B.C.)
Geocentric Model


The Greeks believed in a geocentric
universe, in which the known planets
and the Sun revolved around the Earth.


The path of an object as it goes around
another object in space is called an orbit.



Beyond the planets was an invisible
sphere on which the stars traveled daily
around Earth  celestial sphere



The Greeks attempted to explain the
movements of all celestial bodies in space
by using this geocentric model.
Ptolemaic System


The Greek
astronomer, Ptolemy, presented a
geocentric model of the universe
called the Ptolemaic System, with
fixed stars in the background.
 Although Ptolemy’s

theory was
wrong in that the planets do not
orbit Earth, it was able to account
for the planets’ apparent
motions, which he called epicycles.

Ptolemy (90-168 A.D.)
Geocentric Universe


The idea that the earth is at
the center of the universe and
all things fall around her is the
simplest and longest lasting
universal view that we have
had.
What the Geocentric Universe is made
of
Sun
 Moon
 Stars
 5 Planets


 Mercury
 Venus

 Mars
 Jupiter
 Saturn

 How

did they
discover the
existence of
these planets?
Assumptions about the
Universe
1. The earth is the center of all
motion.
 2. The earth does not move.
 3. The earth is flat.
 4. Planets move in circular orbit.
 5. Stars are immutable.

Heliocentric Model




The first Greek astronomer to
propose a heliocentric universe, in
which Earth and the other planets
orbit the Sun, was Aristarchus.

Though much evidence was
provided to support a heliocentric
universe, the Earth-centered
(geocentric) view dominated
Western thought for 2000 years.

Aristarchus (312-230
B.C.)
The Birth of Modern Astronomy


After Ptolemy, very few advances
were made in astronomy.



The first great astronomer to
emerge after the Middle Ages was
a man from Poland named
Nicolaus Copernicus.



He believed the Earth was a
planet, just like the other 5 known
at the time, and supported the
heliocentric model of the universe.

Copernicus (1473-1543)
Father of Modern
Astronomy
The Birth of Modern Astronomy


After the death of Copernicus came a
Danish astronomer, Tycho Brahe.



Brahe became interested in astronomy
from viewing the astonishing effects of a
solar eclipse.



Had an observatory built where he
designed instruments in order to view and
measure locations of celestial bodies.


Still believed in a geocentric universe based
on his observations of stars.



Gained recognition for being extremely
precise on his observations.

Brahe (1546-1601)
Summary of Brahe's
Contributions


He made the most precise observations
that had yet been made by devising the
best instruments available before the
invention of the telescope.



His observations of planetary
motion, particularly that of
Mars, provided the crucial data for later
astronomers like Kepler to construct our
present model of the solar system.
The Birth of Modern Astronomy


Before Brahe died he hired an
assistant, Johannes Kepler, who
carried on and inherited all of Brahe’s
works.




Didn’t agree Brahe’s view of a
geocentric universe.

Discovered 3 Laws of Planetary
Motion:
1. The path each planet takes around the
Sun is oval-shaped and known as an
ellipse.

Kepler (1571-1630)
The Birth of Modern Astronomy
2. Each planet revolves so an imaginary line connecting
it to the Sun sweeps over equal area in equal time
intervals. A planet travels faster when it is closer to
the Sun and slower when it is farther from the Sun.
The Birth of Modern Astronomy
3. The square of a planet’s orbital period (the time it
takes to orbit the Sun) is proportional to the cube of
its average distance to the Sun:
The orbital period of revolution (P) is
measured in Earth years. The planet’s
distance (a) to the sun is expressed in
astronomical units (AU’s), which is
the average distance between the
Earth and the Sun, approximately 150
million km. or 93 million miles.
The Birth of Modern Astronomy


Galileo Galilei was a great Italian
scientist during the Renaissance.


His most important contributions were
his descriptions of the behavior of
moving objects.



Everything prior to Galileo was studied
and examined without a telescope.



He constructed his own telescope and
used it to study the sky, making many
important discoveries supporting
Copernicus’s view of the universe.

Galileo (1564-1642)
Galileo: the Telescope &
the Laws of Dynamics




Galileo Galilei (1564-1642)
was a pivotal figure in the
development of modern
astronomy, both because of
his contributions directly to
astronomy, and because of
his work in physics and its
relation to astronomy.
He provided the crucial
observations that proved the
Copernican hypothesis, and
also laid the foundations for a
correct understanding of how
objects moved on the surface
of the earth (dynamics) and
of gravity.
The Telescope


Galileo did not invent
the telescope (Dutch
spectacle makers
receive that credit –
Hans Leppershey), but
he was the first to use
the telescope to study
the heavens
systematically.



It is said that what
Galileo saw was so
disturbing for some
officials of the
Church that they
refused to even look
through his
telescope; they
reasoned that the
Devil was capable of
making anything
appear in the
telescope, so it was
best not to look
through it.
Sir Isaac Newton and the
Unification of Physics & Astronomy


Sir Isaac Newton
(1642-1727) was by
many standards the
most important figure
in the development of
modern science. Many
would credit him and
Einstein with being the
most original thinkers
in science
Sir Isaac Newton: The
Universal Law of Gravitation


There is a popular story
that Newton was sitting
under an apple tree, an
apple fell on his
head, and he suddenly
thought of the Universal
Law of Gravitation. As in
all such legends, this is
almost certainly not true
in its details, but the story
contains elements of
what actually happened.
Albert Einstein and
the Theory of Relativity


Motion is relative not absolute.



Other striking consequences are
associated with the dependence of space
and time on velocity: at speeds near that
of light, space itself becomes contracted
in the direction of motion and the
passage of time slows. Although these
seem bizarre ideas (because our
everyday experience typically does not
include speeds near that of light), many
experiments indicate that the Special
Theory of Relativity is correct and our
"common sense" (and Newton's laws)
are incorrect near the speed of light.
SUMMARY
Galilean satellites
Earth is the
center of motion

Galileo
Phases of Venus

Earth IS flat
Newton

Earth is does not
move

Einstein

Planets move in
circular orbits

Kepler

Stars are
immutable

Brahe

Universal Law of
Laws of Motion
Gravitation

Theory of Relativity
Laws of Planetary
Motion

Supernova

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Astronomy lesson thursday

  • 2. Early Astronomy  Astronomy is the science studying outer space and the universe.  The “Golden Age” of astronomy was centered in Greece.
  • 3. Early Astronomy  The Greeks took measurements of distant objects such as the Sun and the moon.  Famous Greek philosopher, Aristotle, conclude d Earth is round because it always cast a curved shadow on the moon.  Another Greek astronomer, Hipparchus, deter mined the location of almost Aristotle (384-322 B.C.) Hipparchus (190-120 B.C.)
  • 4. Geocentric Model  The Greeks believed in a geocentric universe, in which the known planets and the Sun revolved around the Earth.  The path of an object as it goes around another object in space is called an orbit.  Beyond the planets was an invisible sphere on which the stars traveled daily around Earth  celestial sphere  The Greeks attempted to explain the movements of all celestial bodies in space by using this geocentric model.
  • 5. Ptolemaic System  The Greek astronomer, Ptolemy, presented a geocentric model of the universe called the Ptolemaic System, with fixed stars in the background.  Although Ptolemy’s theory was wrong in that the planets do not orbit Earth, it was able to account for the planets’ apparent motions, which he called epicycles. Ptolemy (90-168 A.D.)
  • 6. Geocentric Universe  The idea that the earth is at the center of the universe and all things fall around her is the simplest and longest lasting universal view that we have had.
  • 7. What the Geocentric Universe is made of Sun  Moon  Stars  5 Planets   Mercury  Venus  Mars  Jupiter  Saturn  How did they discover the existence of these planets?
  • 8. Assumptions about the Universe 1. The earth is the center of all motion.  2. The earth does not move.  3. The earth is flat.  4. Planets move in circular orbit.  5. Stars are immutable. 
  • 9. Heliocentric Model   The first Greek astronomer to propose a heliocentric universe, in which Earth and the other planets orbit the Sun, was Aristarchus. Though much evidence was provided to support a heliocentric universe, the Earth-centered (geocentric) view dominated Western thought for 2000 years. Aristarchus (312-230 B.C.)
  • 10. The Birth of Modern Astronomy  After Ptolemy, very few advances were made in astronomy.  The first great astronomer to emerge after the Middle Ages was a man from Poland named Nicolaus Copernicus.  He believed the Earth was a planet, just like the other 5 known at the time, and supported the heliocentric model of the universe. Copernicus (1473-1543) Father of Modern Astronomy
  • 11. The Birth of Modern Astronomy  After the death of Copernicus came a Danish astronomer, Tycho Brahe.  Brahe became interested in astronomy from viewing the astonishing effects of a solar eclipse.  Had an observatory built where he designed instruments in order to view and measure locations of celestial bodies.  Still believed in a geocentric universe based on his observations of stars.  Gained recognition for being extremely precise on his observations. Brahe (1546-1601)
  • 12. Summary of Brahe's Contributions  He made the most precise observations that had yet been made by devising the best instruments available before the invention of the telescope.  His observations of planetary motion, particularly that of Mars, provided the crucial data for later astronomers like Kepler to construct our present model of the solar system.
  • 13. The Birth of Modern Astronomy  Before Brahe died he hired an assistant, Johannes Kepler, who carried on and inherited all of Brahe’s works.   Didn’t agree Brahe’s view of a geocentric universe. Discovered 3 Laws of Planetary Motion: 1. The path each planet takes around the Sun is oval-shaped and known as an ellipse. Kepler (1571-1630)
  • 14. The Birth of Modern Astronomy 2. Each planet revolves so an imaginary line connecting it to the Sun sweeps over equal area in equal time intervals. A planet travels faster when it is closer to the Sun and slower when it is farther from the Sun.
  • 15.
  • 16. The Birth of Modern Astronomy 3. The square of a planet’s orbital period (the time it takes to orbit the Sun) is proportional to the cube of its average distance to the Sun: The orbital period of revolution (P) is measured in Earth years. The planet’s distance (a) to the sun is expressed in astronomical units (AU’s), which is the average distance between the Earth and the Sun, approximately 150 million km. or 93 million miles.
  • 17. The Birth of Modern Astronomy  Galileo Galilei was a great Italian scientist during the Renaissance.  His most important contributions were his descriptions of the behavior of moving objects.  Everything prior to Galileo was studied and examined without a telescope.  He constructed his own telescope and used it to study the sky, making many important discoveries supporting Copernicus’s view of the universe. Galileo (1564-1642)
  • 18. Galileo: the Telescope & the Laws of Dynamics   Galileo Galilei (1564-1642) was a pivotal figure in the development of modern astronomy, both because of his contributions directly to astronomy, and because of his work in physics and its relation to astronomy. He provided the crucial observations that proved the Copernican hypothesis, and also laid the foundations for a correct understanding of how objects moved on the surface of the earth (dynamics) and of gravity.
  • 19.
  • 20. The Telescope  Galileo did not invent the telescope (Dutch spectacle makers receive that credit – Hans Leppershey), but he was the first to use the telescope to study the heavens systematically.  It is said that what Galileo saw was so disturbing for some officials of the Church that they refused to even look through his telescope; they reasoned that the Devil was capable of making anything appear in the telescope, so it was best not to look through it.
  • 21. Sir Isaac Newton and the Unification of Physics & Astronomy  Sir Isaac Newton (1642-1727) was by many standards the most important figure in the development of modern science. Many would credit him and Einstein with being the most original thinkers in science
  • 22. Sir Isaac Newton: The Universal Law of Gravitation  There is a popular story that Newton was sitting under an apple tree, an apple fell on his head, and he suddenly thought of the Universal Law of Gravitation. As in all such legends, this is almost certainly not true in its details, but the story contains elements of what actually happened.
  • 23. Albert Einstein and the Theory of Relativity  Motion is relative not absolute.  Other striking consequences are associated with the dependence of space and time on velocity: at speeds near that of light, space itself becomes contracted in the direction of motion and the passage of time slows. Although these seem bizarre ideas (because our everyday experience typically does not include speeds near that of light), many experiments indicate that the Special Theory of Relativity is correct and our "common sense" (and Newton's laws) are incorrect near the speed of light.
  • 24. SUMMARY Galilean satellites Earth is the center of motion Galileo Phases of Venus Earth IS flat Newton Earth is does not move Einstein Planets move in circular orbits Kepler Stars are immutable Brahe Universal Law of Laws of Motion Gravitation Theory of Relativity Laws of Planetary Motion Supernova