SlideShare a Scribd company logo
1 of 48
The Copernican Revolution
The Beginning of Modern Astronomy
The 15th Century
• In 1453 Ottoman Turks overrun
Constantinople.
• Romans flee west into Europe and take
books with them.
• This end the Middle Ages.
• Most people cannot read or write and
generally believe that:
The 15th Century Astronomy
• Earth is stationary sphere at the center of heaven.
It’s habitable surface is a flat circle with Jerusalem
at it’s center.
• Stars and planets made of a perfect substance
called aether a 5th
heavenly element.
• Moon, sun and stars held in place by invisible
crystalline spheres.
• Heaven is its own sphere above the stars.
• Hell is where Satan lives and is below the
habitable surface of earth.
99 Years That Shook Astronomy
Recall that astronomical models need to explain the
following observations of the sky:
1. Why does the celestial sphere appear to move east to west
each day (diurnal motion)?
2. Why do the Sun and planets appear to move eastward
along the Zodiac?
3. How can planetary alignments such as oppositions and
conjunctions be explained?
4. Why are Mercury and Venus never seen opposite of the
Sun in the sky?
5. Why do planets have retrograde motion that causes them
to appear to go backwards?
Recall Ptolemy’s Model
Nicholas Copernicus (1473-
1543)Polish Catholic Cleric
Observed night sky from
an observation tower.
Trying to solve the calendar
problem.
Suggested a Sun centered Universe
in a book titled De Revolutionibus,
which was not published until
the year he died.
NOTE: He was well educated
and had read Greek astronomy.
Copernican Model
• Heliocentric Universe
• De Revolutionibus
Orbiun Celestium (On
the Revolutions of the
Heavenly Spheres)
• Idea was opposed by
the Catholic Church
(recall Cosmas flat
earth and pagans
round earth.)
http://es.rice.edu/ES/humsoc/Galileo/Images/Astro/Conceptions/copernican_universe.gif
Copernican Model
Copernican Model Explained
• Earth’s rotation caused daily motion from east to
west.
• Mercury and Venus were inferior planets, which
explained why they are always seen near the Sun.
• Sun’s annual motion along the ecliptic (Zodiac)
was caused by Earth’s orbital motion (this one was
difficult to accept.)
• Retrograde motion was a natural phenomenon of
one planet passing another planet as they orbited
the Sun.
Retrograde
Motion
As a faster moving planet
overtakes and passes a
slower moving superior
planet the superior planet
appears to move backwards
as you pass by it.
Copernican Model
Why believe Copernican model?
• Ptolemy’s model had worked for 1500 years.
• Ptolemy’s model provided a metaphor of the earth
and humans living at the center of God’s creation.
• Copernicus did not prove that the Earth orbited the
Sun.
• Copernican model did not predict the positions of
planets any better than Ptolemy’s model.
Occam’s Razor
• William of Occam England, 14th
Century
• "If you have two theories which both explain the observed
facts then you should use the simplest until more evidence
comes along“
• "The simplest explanation for some phenomenon is more
likely to be accurate than more complicated explanations.“
• KISS (instructor’s editorial comment)
Copernican Model
Why believe Copernican model?
• It was aesthetically more pleasing.
• It was more simple.
• It explained complex motions as naturally
occurring.
SN 1572, Tycho's Supernova
''On the 11th day of November in the evening after sunset, I was
contemplating the stars in a clear sky. I noticed that a new and
unusual star, surpassing the other stars in brilliancy, was shining
almost directly above my head; and since I had, from boyhood,
known all the stars of the heavens perfectly, it was quite evident to
me that there had never been any star in that place of the sky, even
the smallest, to say nothing of a star so conspicuous and bright as
this. I was so astonished of this sight that I was not ashamed to
doubt the trustworthiness of my own eyes. But when I observed
that others, on having the place pointed out to them, could see that
there was really a star there, I had no further doubts. A miracle
indeed, one that has never been previously seen before our time, in
any age since the beginning of the world.''
http://www.seds.org/~spider/spider/Vars/sn1572.html
SN 1572, Tycho's
Supernova
http://www.seds.org/~spider/spider/Vars/sn1572.html
http://www.solstation.com/x-objects/tycho-s.htm
This showed him the universe
was not changeless and it shook
his very core beliefs.
Tycho Brahe (1546-1607)
• Supernova caused him to
do research astronomy
• Danish nobleman
• Keen eyed observer
• Had a gold nose.
• Built an observatory
named Uraniborg on the
Danish island of Hveen.
Tycho’s Observatory
• Used for 20 years.
• Largest quadrants in the
world.
• Made the most accurate
observation’s of planetary
and star positions (+ 1
arcminute.)
• 1 arcminute is 1/60 of a
degree.
Johannes Kepler (1571-1630)
• German Lutheran
theologian &
mathematician.
• Sought to prove
Copernican model correct.
• He saw the model
representing God in the
center of the universe with
his creation surrounding
him.
Kepler’s Model
• He believed that God
created the universe using
the language of geometry.
• Used the 5 regular solids
with equal sized faces to
hold up the celestial
spheres.
• That explained why there
were only 6 planets.
• TOTALLY WRONG, but
he believed in it until he
died.
Kepler & Tycho
• Kepler was exiled from Graz for being
Lutheran.
• Tycho had left Uraniborg for Prague.
• Tycho invited Kepler to join him Prague.
• A strained relationship and collaboration
developed. (They did not like each other!)
Kepler & Tycho
• Kepler needed Tycho’s precise observations
to prove his model of nested spheres.
• Tycho needed Kepler’s theoretical and
mathematical mind to prove Tycho’s model
to be correct (a strange combination of an
Earth centered and Copernican model that
never gained favor.)
SN 1604, Kepler's Supernova
http://www.seds.org/~spider/spider/Vars/sn1604.html
http://en.wikipedia.org/wiki/Johannes_Kepler
A few years before Tycho died
another supernova was observed
by Kepler in constellation of
Ophiuchus on October 17th
1604.
It had been observed by others as
early as Oct. 4th
.
(Last known supernova in Milky Way.)
Kepler & Tycho
• After Tycho’s death, and many court battles with his
relatives, Kepler gained access to Tycho’s data.
• Tycho had always claimed that the data for Mars was the
most difficult to reconcile with any theory.
• Working on Mars caused Kepler to abandon perfect
circular orbits and replace them with elliptical orbits.
Kepler’s Laws
1st
Law
• Planets orbit the Sun
in elliptical paths with
the Sun at one focus.
Kepler & Ptolemy
Kepler’s Laws
2nd
Law
• Law of Areas
• A line connecting the Sun
and a planet sweeps out
equal areas in equal times.
• This means that a planet
moves fastest when it is
closest to the Sun.
Kepler’s Laws
3rd Law
• The Harmonic Law
• P2
= a3
where
– P = orbital period in years
– a = semi-major axis in Astronomical Units (au).
An au = average distance between Earth and Sun
~ 93,000,000 miles or 150,000,000 Km.
Kepler’s Laws
3rd Law
• Example Calculation for Jupiter
• a = 5.2 au’s
• P2
= a3
substituting for a
• P2
= (5.2)3
= 5.2 x 5.2 x 5.2 = 140.6
• Take square root of 140.6
• P = 11.86 years
Review of Kepler’s Laws
1st
Law 2nd
Law 3rd
Law
Galileo Galilei (1564-1642)
• The father of Physics
• First person to point a
telescope at the night sky.
• In 1610 he wrote The
Starry Messenger in
which he published his
observations.
Galileo’s Telescopic Discoveries
• Craters on Moon
• Sunspots
• Moon’s of Jupiter
• Phases of Venus
All of these data were
used as evidence for
the Copernican
Model.
Replica of Galileo’s telescope from
http://www.museum.vic.gov.au/scidiscovery/scientists/galileo.asp
Craters on the Moon
• Moon is NOT
perfect
• It has craters
• It has mountains
http://www.hao.ucar.edu/public/education/sp/images/galileo.html
Sunspots
• Sun is NOT perfect.
• It has dark spots.
• What are sunspots?
• The Sun may rotate,
which implies the
Earth may rotate.
http://www.sunblock99.org.uk/sb99/people/KMacpher/first_obs.html
Moons of Jupiter
• January 7-15, 1610
• These moon’s do not
revolve around the
Earth or the Sun!
• They form a miniature
solar system of their
own.
Phases
of
Venus
Isaac Newton (1642-1727)
• Develops Laws of Motion
• Develops idea of gravity
to get Edmund Halley off
his back.
• Halley paid to publish
Mathematical Principles
of Natural Philosophy.
• Derived Kepler’s three
laws of planetary motion
using laws of motion and
gravity.
http://www.hao.ucar.edu/public/education/sp/images/newton.html
Newton’s Laws
1st
Law
• Law of Inertia
• A body at rest will
remain at rest, and a
body in motion will
remain in motion,
unless acted upon by
an unbalanced force.
Newton’s Laws
2nd Law
• An acceleration is caused by an unbalanced
force acting on an object and is directly
proportional to the magnitude (strength) of
the force applied in the direction of the
force.
• a α F
Newton’s Laws
2nd Law
• The acceleration of an object being acted
upon by an unbalanced force is inversely
proportional to the object’s mass, m.
• a α 1/m
Newton’s Laws
2nd Law
• Force Law
• F = ma
• Force units are,
F = (kg)(m/s2
) = N ( 1
Newton).
• 1N ~ the weight of an
apple.
Newton’s Laws
3rd Law
• Action and Reaction
• For every action there is an
equal and opposite reaction.
• F1 = -F2
• m1a1 = -m2a2
• Forces act in opposite
directions on different
objects.
Newton’s Laws
Examples of 3rd Law
Gravity
Every object in the universe appears to attract every other
object in the universe with a force that is directly
proportional to the product of their masses and inversely
proportional to the square of the distances between them.
• F α (m1m2)/r2
• F = G(m1m2)/r2
, where G is the gravitational constant.
• G = 6.67x10-11
Nm2
/kg2
The Gravity of the Situation
A quick lesson on the Nature of Science
Is it the
Law of Gravity
or the
Theory of Gravity?
Newton’s Laws
2nd
Law
Mass & Weight
• Mass is not equal to
weight.
• Weight is force of
gravity acting on a
mass.
• F = ma = mg.
• W = mg.
• W = (1.0kg)(9.8m/s2
)
= 9.8N.
Orbital
Motion
and
Freefall
Resources
Chaisson and McMillian, (2002). Astronomy Today
(4th
Ed.)
Hewitt, (1998). Conceptual Physics (8th
Ed.)
http://www.usoe.k12.ut.us/curr/science/sciber00/8th/forces/s
Shipman, Wilson, and Todd, (2003). An Introduction
to Physical Science (10th
Edition).

More Related Content

What's hot

Science and technonology and nation building
Science and technonology and nation building  Science and technonology and nation building
Science and technonology and nation building donna ruth talo
 
Early model of the Universe
Early model of the UniverseEarly model of the Universe
Early model of the UniverseJerome Bigael
 
science, technology and society
science, technology and societyscience, technology and society
science, technology and societyMerlyn Denesia
 
External and internal criticisms
External and internal criticismsExternal and internal criticisms
External and internal criticismsmyboyfriend10
 
Physical science chapter1 for shs
Physical science chapter1 for shsPhysical science chapter1 for shs
Physical science chapter1 for shsJimnaira Abanto
 
Site of-first-mass-in-the-philippines history-1-4
Site of-first-mass-in-the-philippines history-1-4Site of-first-mass-in-the-philippines history-1-4
Site of-first-mass-in-the-philippines history-1-4Richard Decilio
 
Early Models of the Universe
Early Models of the UniverseEarly Models of the Universe
Early Models of the UniverseHanna Elise
 
MOTION (The Restless Universe)
MOTION (The Restless Universe)MOTION (The Restless Universe)
MOTION (The Restless Universe)Hanna Elise
 
Mathematics in the Modern World Lecture 1
Mathematics in the Modern World Lecture 1Mathematics in the Modern World Lecture 1
Mathematics in the Modern World Lecture 1AnnaClariceYanday
 
Aristotle vs. Galileo
Aristotle vs. GalileoAristotle vs. Galileo
Aristotle vs. GalileoHanna Elise
 
Scientific revolution lesson ppt
Scientific revolution lesson pptScientific revolution lesson ppt
Scientific revolution lesson pptGreg Sill
 
Nicolaus copernicus
Nicolaus copernicusNicolaus copernicus
Nicolaus copernicusryedevaught
 
Lesson 2 intellectual revolutions that defined society
Lesson 2 intellectual revolutions that defined societyLesson 2 intellectual revolutions that defined society
Lesson 2 intellectual revolutions that defined societydonna ruth talo
 

What's hot (20)

bsp-sts pt2
bsp-sts pt2bsp-sts pt2
bsp-sts pt2
 
Science and technonology and nation building
Science and technonology and nation building  Science and technonology and nation building
Science and technonology and nation building
 
Early model of the Universe
Early model of the UniverseEarly model of the Universe
Early model of the Universe
 
science, technology and society
science, technology and societyscience, technology and society
science, technology and society
 
External and internal criticisms
External and internal criticismsExternal and internal criticisms
External and internal criticisms
 
Controversies in philippine history
Controversies in philippine historyControversies in philippine history
Controversies in philippine history
 
Physical science chapter1 for shs
Physical science chapter1 for shsPhysical science chapter1 for shs
Physical science chapter1 for shs
 
Geocentric Model
Geocentric ModelGeocentric Model
Geocentric Model
 
M1_Lesson 3_Brahe's Innovation.pptx
M1_Lesson 3_Brahe's Innovation.pptxM1_Lesson 3_Brahe's Innovation.pptx
M1_Lesson 3_Brahe's Innovation.pptx
 
Site of-first-mass-in-the-philippines history-1-4
Site of-first-mass-in-the-philippines history-1-4Site of-first-mass-in-the-philippines history-1-4
Site of-first-mass-in-the-philippines history-1-4
 
Filipino values
Filipino valuesFilipino values
Filipino values
 
Early Models of the Universe
Early Models of the UniverseEarly Models of the Universe
Early Models of the Universe
 
MOTION (The Restless Universe)
MOTION (The Restless Universe)MOTION (The Restless Universe)
MOTION (The Restless Universe)
 
Mathematics in the Modern World Lecture 1
Mathematics in the Modern World Lecture 1Mathematics in the Modern World Lecture 1
Mathematics in the Modern World Lecture 1
 
Aristotle vs. Galileo
Aristotle vs. GalileoAristotle vs. Galileo
Aristotle vs. Galileo
 
Scientific revolution lesson ppt
Scientific revolution lesson pptScientific revolution lesson ppt
Scientific revolution lesson ppt
 
Nicolaus copernicus
Nicolaus copernicusNicolaus copernicus
Nicolaus copernicus
 
Lesson 2 intellectual revolutions that defined society
Lesson 2 intellectual revolutions that defined societyLesson 2 intellectual revolutions that defined society
Lesson 2 intellectual revolutions that defined society
 
Physical Self
Physical Self Physical Self
Physical Self
 
The-Information-Age.pptx
The-Information-Age.pptxThe-Information-Age.pptx
The-Information-Age.pptx
 

Similar to Copernican revolution

Discovering the Universe - Gravitiation
Discovering the Universe - GravitiationDiscovering the Universe - Gravitiation
Discovering the Universe - Gravitiationbrycetbolin
 
Johannes kepler nomination
Johannes kepler nominationJohannes kepler nomination
Johannes kepler nominationdom vin
 
Astonishing Astronomy 101 - Chapter 2
Astonishing Astronomy 101 - Chapter 2Astonishing Astronomy 101 - Chapter 2
Astonishing Astronomy 101 - Chapter 2Don R. Mueller, Ph.D.
 
Professor’s Questions Set 2Provide comprehensive answers to th.docx
Professor’s Questions Set 2Provide comprehensive answers to th.docxProfessor’s Questions Set 2Provide comprehensive answers to th.docx
Professor’s Questions Set 2Provide comprehensive answers to th.docxwkyra78
 
Models of astronomical phenomena
Models of astronomical phenomenaModels of astronomical phenomena
Models of astronomical phenomenaCher Jessa
 
Johannes Kepler's Contribution in Science.pptx
Johannes Kepler's Contribution in Science.pptxJohannes Kepler's Contribution in Science.pptx
Johannes Kepler's Contribution in Science.pptxJonathanParaisoCruz
 
99 years modern astronomy
99 years modern astronomy99 years modern astronomy
99 years modern astronomyElaine Espiel
 
Brief history of time episode 1
Brief history of time episode 1Brief history of time episode 1
Brief history of time episode 1UmarRahman7
 
Asma Said 03 lecture outline
Asma Said 03 lecture outlineAsma Said 03 lecture outline
Asma Said 03 lecture outlineAsma Said,PhD
 
Lesson 1 history of astronomy3
Lesson 1  history of astronomy3Lesson 1  history of astronomy3
Lesson 1 history of astronomy3Adrian
 
Introduction to cosmology
Introduction to cosmologyIntroduction to cosmology
Introduction to cosmologyChristian Costa
 
Math In Space: Planetary Orbits
Math In Space: Planetary OrbitsMath In Space: Planetary Orbits
Math In Space: Planetary OrbitsGregory Tewksbury
 

Similar to Copernican revolution (20)

4.6- The Wanderers ves 7.pptx
4.6- The Wanderers ves 7.pptx4.6- The Wanderers ves 7.pptx
4.6- The Wanderers ves 7.pptx
 
4.6- The Wanderers ves 7.pptx
4.6- The Wanderers ves 7.pptx4.6- The Wanderers ves 7.pptx
4.6- The Wanderers ves 7.pptx
 
4.6- The Wanderers ves 7.pptx
4.6- The Wanderers ves 7.pptx4.6- The Wanderers ves 7.pptx
4.6- The Wanderers ves 7.pptx
 
astronomers.ppt
astronomers.pptastronomers.ppt
astronomers.ppt
 
Discovering the Universe - Gravitiation
Discovering the Universe - GravitiationDiscovering the Universe - Gravitiation
Discovering the Universe - Gravitiation
 
Johannes kepler nomination
Johannes kepler nominationJohannes kepler nomination
Johannes kepler nomination
 
Gravitation 1
Gravitation 1Gravitation 1
Gravitation 1
 
Astonishing Astronomy 101 - Chapter 2
Astonishing Astronomy 101 - Chapter 2Astonishing Astronomy 101 - Chapter 2
Astonishing Astronomy 101 - Chapter 2
 
Helio vs geo 2 ge notes
Helio vs geo 2 ge notesHelio vs geo 2 ge notes
Helio vs geo 2 ge notes
 
A. history of astronomy
A. history of astronomyA. history of astronomy
A. history of astronomy
 
Professor’s Questions Set 2Provide comprehensive answers to th.docx
Professor’s Questions Set 2Provide comprehensive answers to th.docxProfessor’s Questions Set 2Provide comprehensive answers to th.docx
Professor’s Questions Set 2Provide comprehensive answers to th.docx
 
Models of astronomical phenomena
Models of astronomical phenomenaModels of astronomical phenomena
Models of astronomical phenomena
 
ASTRONOMY_ PDF.pdf
ASTRONOMY_ PDF.pdfASTRONOMY_ PDF.pdf
ASTRONOMY_ PDF.pdf
 
Johannes Kepler's Contribution in Science.pptx
Johannes Kepler's Contribution in Science.pptxJohannes Kepler's Contribution in Science.pptx
Johannes Kepler's Contribution in Science.pptx
 
99 years modern astronomy
99 years modern astronomy99 years modern astronomy
99 years modern astronomy
 
Brief history of time episode 1
Brief history of time episode 1Brief history of time episode 1
Brief history of time episode 1
 
Asma Said 03 lecture outline
Asma Said 03 lecture outlineAsma Said 03 lecture outline
Asma Said 03 lecture outline
 
Lesson 1 history of astronomy3
Lesson 1  history of astronomy3Lesson 1  history of astronomy3
Lesson 1 history of astronomy3
 
Introduction to cosmology
Introduction to cosmologyIntroduction to cosmology
Introduction to cosmology
 
Math In Space: Planetary Orbits
Math In Space: Planetary OrbitsMath In Space: Planetary Orbits
Math In Space: Planetary Orbits
 

More from Dr Robert Craig PhD

Hofstra Living environment Dr Rob
Hofstra Living environment Dr RobHofstra Living environment Dr Rob
Hofstra Living environment Dr RobDr Robert Craig PhD
 
Chapter 2-Your text book ves 5.pptx
Chapter 2-Your text book ves 5.pptxChapter 2-Your text book ves 5.pptx
Chapter 2-Your text book ves 5.pptxDr Robert Craig PhD
 
Brown dwarfs and planets jaslyn.pdf
Brown dwarfs and planets jaslyn.pdfBrown dwarfs and planets jaslyn.pdf
Brown dwarfs and planets jaslyn.pdfDr Robert Craig PhD
 
Day 1 Martin file from syllabus ves 5.pptx
Day 1 Martin file from syllabus ves 5.pptxDay 1 Martin file from syllabus ves 5.pptx
Day 1 Martin file from syllabus ves 5.pptxDr Robert Craig PhD
 
Astronomy chapter 1 power point.pptx
Astronomy chapter 1 power point.pptxAstronomy chapter 1 power point.pptx
Astronomy chapter 1 power point.pptxDr Robert Craig PhD
 
5Page43 how to classify stars parkslope heard from Annie.pdf
5Page43 how to classify stars parkslope  heard from Annie.pdf5Page43 how to classify stars parkslope  heard from Annie.pdf
5Page43 how to classify stars parkslope heard from Annie.pdfDr Robert Craig PhD
 
1-D Kinematics AP Lab Graphing.docx
1-D Kinematics AP Lab Graphing.docx1-D Kinematics AP Lab Graphing.docx
1-D Kinematics AP Lab Graphing.docxDr Robert Craig PhD
 
03 - Average Rates of Changec Cameron 1 Sara Hill.pdf
03 - Average Rates of Changec Cameron 1 Sara Hill.pdf03 - Average Rates of Changec Cameron 1 Sara Hill.pdf
03 - Average Rates of Changec Cameron 1 Sara Hill.pdfDr Robert Craig PhD
 
5.4- Measuring the Earth with Eratosthenes. Ves 2.pdf
5.4- Measuring the Earth with Eratosthenes. Ves 2.pdf5.4- Measuring the Earth with Eratosthenes. Ves 2.pdf
5.4- Measuring the Earth with Eratosthenes. Ves 2.pdfDr Robert Craig PhD
 
chapter 2 redone parkslope ves 4.pdf
chapter 2 redone parkslope ves 4.pdfchapter 2 redone parkslope ves 4.pdf
chapter 2 redone parkslope ves 4.pdfDr Robert Craig PhD
 
season_path_of_the_sun_and_latitude.pdf
season_path_of_the_sun_and_latitude.pdfseason_path_of_the_sun_and_latitude.pdf
season_path_of_the_sun_and_latitude.pdfDr Robert Craig PhD
 

More from Dr Robert Craig PhD (20)

Hofstra Living environment Dr Rob
Hofstra Living environment Dr RobHofstra Living environment Dr Rob
Hofstra Living environment Dr Rob
 
pdf (4) 4.pdf
pdf (4) 4.pdfpdf (4) 4.pdf
pdf (4) 4.pdf
 
Mastering_Assignments.pdf.pdf
Mastering_Assignments.pdf.pdfMastering_Assignments.pdf.pdf
Mastering_Assignments.pdf.pdf
 
Lecture3.pdf
Lecture3.pdfLecture3.pdf
Lecture3.pdf
 
Lecture2.pdf
Lecture2.pdfLecture2.pdf
Lecture2.pdf
 
Lecture0.pdf
Lecture0.pdfLecture0.pdf
Lecture0.pdf
 
lecture 11 of 12 ves 1.pptx
lecture 11 of 12 ves 1.pptxlecture 11 of 12 ves 1.pptx
lecture 11 of 12 ves 1.pptx
 
Chapter 2-Your text book ves 5.pptx
Chapter 2-Your text book ves 5.pptxChapter 2-Your text book ves 5.pptx
Chapter 2-Your text book ves 5.pptx
 
Brown dwarfs and planets jaslyn.pdf
Brown dwarfs and planets jaslyn.pdfBrown dwarfs and planets jaslyn.pdf
Brown dwarfs and planets jaslyn.pdf
 
Day 1 Martin file from syllabus ves 5.pptx
Day 1 Martin file from syllabus ves 5.pptxDay 1 Martin file from syllabus ves 5.pptx
Day 1 Martin file from syllabus ves 5.pptx
 
Astronomy chapter 1 power point.pptx
Astronomy chapter 1 power point.pptxAstronomy chapter 1 power point.pptx
Astronomy chapter 1 power point.pptx
 
5Page43 how to classify stars parkslope heard from Annie.pdf
5Page43 how to classify stars parkslope  heard from Annie.pdf5Page43 how to classify stars parkslope  heard from Annie.pdf
5Page43 how to classify stars parkslope heard from Annie.pdf
 
1-D Kinematics AP Lab Graphing.docx
1-D Kinematics AP Lab Graphing.docx1-D Kinematics AP Lab Graphing.docx
1-D Kinematics AP Lab Graphing.docx
 
03 - Average Rates of Changec Cameron 1 Sara Hill.pdf
03 - Average Rates of Changec Cameron 1 Sara Hill.pdf03 - Average Rates of Changec Cameron 1 Sara Hill.pdf
03 - Average Rates of Changec Cameron 1 Sara Hill.pdf
 
5.4- Measuring the Earth with Eratosthenes. Ves 2.pdf
5.4- Measuring the Earth with Eratosthenes. Ves 2.pdf5.4- Measuring the Earth with Eratosthenes. Ves 2.pdf
5.4- Measuring the Earth with Eratosthenes. Ves 2.pdf
 
Physics chapter 1.docx
Physics chapter 1.docxPhysics chapter 1.docx
Physics chapter 1.docx
 
chapter 2 redone parkslope ves 4.pdf
chapter 2 redone parkslope ves 4.pdfchapter 2 redone parkslope ves 4.pdf
chapter 2 redone parkslope ves 4.pdf
 
season_path_of_the_sun_and_latitude.pdf
season_path_of_the_sun_and_latitude.pdfseason_path_of_the_sun_and_latitude.pdf
season_path_of_the_sun_and_latitude.pdf
 
phys40115050-course-outline.pdf
phys40115050-course-outline.pdfphys40115050-course-outline.pdf
phys40115050-course-outline.pdf
 
Phy100sp20_Lec2.pdf
Phy100sp20_Lec2.pdfPhy100sp20_Lec2.pdf
Phy100sp20_Lec2.pdf
 

Recently uploaded

This PowerPoint helps students to consider the concept of infinity.
This PowerPoint helps students to consider the concept of infinity.This PowerPoint helps students to consider the concept of infinity.
This PowerPoint helps students to consider the concept of infinity.christianmathematics
 
ICT Role in 21st Century Education & its Challenges.pptx
ICT Role in 21st Century Education & its Challenges.pptxICT Role in 21st Century Education & its Challenges.pptx
ICT Role in 21st Century Education & its Challenges.pptxAreebaZafar22
 
UGC NET Paper 1 Mathematical Reasoning & Aptitude.pdf
UGC NET Paper 1 Mathematical Reasoning & Aptitude.pdfUGC NET Paper 1 Mathematical Reasoning & Aptitude.pdf
UGC NET Paper 1 Mathematical Reasoning & Aptitude.pdfNirmal Dwivedi
 
SKILL OF INTRODUCING THE LESSON MICRO SKILLS.pptx
SKILL OF INTRODUCING THE LESSON MICRO SKILLS.pptxSKILL OF INTRODUCING THE LESSON MICRO SKILLS.pptx
SKILL OF INTRODUCING THE LESSON MICRO SKILLS.pptxAmanpreet Kaur
 
Application orientated numerical on hev.ppt
Application orientated numerical on hev.pptApplication orientated numerical on hev.ppt
Application orientated numerical on hev.pptRamjanShidvankar
 
On National Teacher Day, meet the 2024-25 Kenan Fellows
On National Teacher Day, meet the 2024-25 Kenan FellowsOn National Teacher Day, meet the 2024-25 Kenan Fellows
On National Teacher Day, meet the 2024-25 Kenan FellowsMebane Rash
 
Jual Obat Aborsi Hongkong ( Asli No.1 ) 085657271886 Obat Penggugur Kandungan...
Jual Obat Aborsi Hongkong ( Asli No.1 ) 085657271886 Obat Penggugur Kandungan...Jual Obat Aborsi Hongkong ( Asli No.1 ) 085657271886 Obat Penggugur Kandungan...
Jual Obat Aborsi Hongkong ( Asli No.1 ) 085657271886 Obat Penggugur Kandungan...ZurliaSoop
 
Unit-IV; Professional Sales Representative (PSR).pptx
Unit-IV; Professional Sales Representative (PSR).pptxUnit-IV; Professional Sales Representative (PSR).pptx
Unit-IV; Professional Sales Representative (PSR).pptxVishalSingh1417
 
The basics of sentences session 3pptx.pptx
The basics of sentences session 3pptx.pptxThe basics of sentences session 3pptx.pptx
The basics of sentences session 3pptx.pptxheathfieldcps1
 
Key note speaker Neum_Admir Softic_ENG.pdf
Key note speaker Neum_Admir Softic_ENG.pdfKey note speaker Neum_Admir Softic_ENG.pdf
Key note speaker Neum_Admir Softic_ENG.pdfAdmir Softic
 
Google Gemini An AI Revolution in Education.pptx
Google Gemini An AI Revolution in Education.pptxGoogle Gemini An AI Revolution in Education.pptx
Google Gemini An AI Revolution in Education.pptxDr. Sarita Anand
 
Salient Features of India constitution especially power and functions
Salient Features of India constitution especially power and functionsSalient Features of India constitution especially power and functions
Salient Features of India constitution especially power and functionsKarakKing
 
Vishram Singh - Textbook of Anatomy Upper Limb and Thorax.. Volume 1 (1).pdf
Vishram Singh - Textbook of Anatomy  Upper Limb and Thorax.. Volume 1 (1).pdfVishram Singh - Textbook of Anatomy  Upper Limb and Thorax.. Volume 1 (1).pdf
Vishram Singh - Textbook of Anatomy Upper Limb and Thorax.. Volume 1 (1).pdfssuserdda66b
 
Kodo Millet PPT made by Ghanshyam bairwa college of Agriculture kumher bhara...
Kodo Millet  PPT made by Ghanshyam bairwa college of Agriculture kumher bhara...Kodo Millet  PPT made by Ghanshyam bairwa college of Agriculture kumher bhara...
Kodo Millet PPT made by Ghanshyam bairwa college of Agriculture kumher bhara...pradhanghanshyam7136
 
TỔNG ÔN TẬP THI VÀO LỚP 10 MÔN TIẾNG ANH NĂM HỌC 2023 - 2024 CÓ ĐÁP ÁN (NGỮ Â...
TỔNG ÔN TẬP THI VÀO LỚP 10 MÔN TIẾNG ANH NĂM HỌC 2023 - 2024 CÓ ĐÁP ÁN (NGỮ Â...TỔNG ÔN TẬP THI VÀO LỚP 10 MÔN TIẾNG ANH NĂM HỌC 2023 - 2024 CÓ ĐÁP ÁN (NGỮ Â...
TỔNG ÔN TẬP THI VÀO LỚP 10 MÔN TIẾNG ANH NĂM HỌC 2023 - 2024 CÓ ĐÁP ÁN (NGỮ Â...Nguyen Thanh Tu Collection
 
Mixin Classes in Odoo 17 How to Extend Models Using Mixin Classes
Mixin Classes in Odoo 17  How to Extend Models Using Mixin ClassesMixin Classes in Odoo 17  How to Extend Models Using Mixin Classes
Mixin Classes in Odoo 17 How to Extend Models Using Mixin ClassesCeline George
 
Python Notes for mca i year students osmania university.docx
Python Notes for mca i year students osmania university.docxPython Notes for mca i year students osmania university.docx
Python Notes for mca i year students osmania university.docxRamakrishna Reddy Bijjam
 
Understanding Accommodations and Modifications
Understanding  Accommodations and ModificationsUnderstanding  Accommodations and Modifications
Understanding Accommodations and ModificationsMJDuyan
 
Food safety_Challenges food safety laboratories_.pdf
Food safety_Challenges food safety laboratories_.pdfFood safety_Challenges food safety laboratories_.pdf
Food safety_Challenges food safety laboratories_.pdfSherif Taha
 
Accessible Digital Futures project (20/03/2024)
Accessible Digital Futures project (20/03/2024)Accessible Digital Futures project (20/03/2024)
Accessible Digital Futures project (20/03/2024)Jisc
 

Recently uploaded (20)

This PowerPoint helps students to consider the concept of infinity.
This PowerPoint helps students to consider the concept of infinity.This PowerPoint helps students to consider the concept of infinity.
This PowerPoint helps students to consider the concept of infinity.
 
ICT Role in 21st Century Education & its Challenges.pptx
ICT Role in 21st Century Education & its Challenges.pptxICT Role in 21st Century Education & its Challenges.pptx
ICT Role in 21st Century Education & its Challenges.pptx
 
UGC NET Paper 1 Mathematical Reasoning & Aptitude.pdf
UGC NET Paper 1 Mathematical Reasoning & Aptitude.pdfUGC NET Paper 1 Mathematical Reasoning & Aptitude.pdf
UGC NET Paper 1 Mathematical Reasoning & Aptitude.pdf
 
SKILL OF INTRODUCING THE LESSON MICRO SKILLS.pptx
SKILL OF INTRODUCING THE LESSON MICRO SKILLS.pptxSKILL OF INTRODUCING THE LESSON MICRO SKILLS.pptx
SKILL OF INTRODUCING THE LESSON MICRO SKILLS.pptx
 
Application orientated numerical on hev.ppt
Application orientated numerical on hev.pptApplication orientated numerical on hev.ppt
Application orientated numerical on hev.ppt
 
On National Teacher Day, meet the 2024-25 Kenan Fellows
On National Teacher Day, meet the 2024-25 Kenan FellowsOn National Teacher Day, meet the 2024-25 Kenan Fellows
On National Teacher Day, meet the 2024-25 Kenan Fellows
 
Jual Obat Aborsi Hongkong ( Asli No.1 ) 085657271886 Obat Penggugur Kandungan...
Jual Obat Aborsi Hongkong ( Asli No.1 ) 085657271886 Obat Penggugur Kandungan...Jual Obat Aborsi Hongkong ( Asli No.1 ) 085657271886 Obat Penggugur Kandungan...
Jual Obat Aborsi Hongkong ( Asli No.1 ) 085657271886 Obat Penggugur Kandungan...
 
Unit-IV; Professional Sales Representative (PSR).pptx
Unit-IV; Professional Sales Representative (PSR).pptxUnit-IV; Professional Sales Representative (PSR).pptx
Unit-IV; Professional Sales Representative (PSR).pptx
 
The basics of sentences session 3pptx.pptx
The basics of sentences session 3pptx.pptxThe basics of sentences session 3pptx.pptx
The basics of sentences session 3pptx.pptx
 
Key note speaker Neum_Admir Softic_ENG.pdf
Key note speaker Neum_Admir Softic_ENG.pdfKey note speaker Neum_Admir Softic_ENG.pdf
Key note speaker Neum_Admir Softic_ENG.pdf
 
Google Gemini An AI Revolution in Education.pptx
Google Gemini An AI Revolution in Education.pptxGoogle Gemini An AI Revolution in Education.pptx
Google Gemini An AI Revolution in Education.pptx
 
Salient Features of India constitution especially power and functions
Salient Features of India constitution especially power and functionsSalient Features of India constitution especially power and functions
Salient Features of India constitution especially power and functions
 
Vishram Singh - Textbook of Anatomy Upper Limb and Thorax.. Volume 1 (1).pdf
Vishram Singh - Textbook of Anatomy  Upper Limb and Thorax.. Volume 1 (1).pdfVishram Singh - Textbook of Anatomy  Upper Limb and Thorax.. Volume 1 (1).pdf
Vishram Singh - Textbook of Anatomy Upper Limb and Thorax.. Volume 1 (1).pdf
 
Kodo Millet PPT made by Ghanshyam bairwa college of Agriculture kumher bhara...
Kodo Millet  PPT made by Ghanshyam bairwa college of Agriculture kumher bhara...Kodo Millet  PPT made by Ghanshyam bairwa college of Agriculture kumher bhara...
Kodo Millet PPT made by Ghanshyam bairwa college of Agriculture kumher bhara...
 
TỔNG ÔN TẬP THI VÀO LỚP 10 MÔN TIẾNG ANH NĂM HỌC 2023 - 2024 CÓ ĐÁP ÁN (NGỮ Â...
TỔNG ÔN TẬP THI VÀO LỚP 10 MÔN TIẾNG ANH NĂM HỌC 2023 - 2024 CÓ ĐÁP ÁN (NGỮ Â...TỔNG ÔN TẬP THI VÀO LỚP 10 MÔN TIẾNG ANH NĂM HỌC 2023 - 2024 CÓ ĐÁP ÁN (NGỮ Â...
TỔNG ÔN TẬP THI VÀO LỚP 10 MÔN TIẾNG ANH NĂM HỌC 2023 - 2024 CÓ ĐÁP ÁN (NGỮ Â...
 
Mixin Classes in Odoo 17 How to Extend Models Using Mixin Classes
Mixin Classes in Odoo 17  How to Extend Models Using Mixin ClassesMixin Classes in Odoo 17  How to Extend Models Using Mixin Classes
Mixin Classes in Odoo 17 How to Extend Models Using Mixin Classes
 
Python Notes for mca i year students osmania university.docx
Python Notes for mca i year students osmania university.docxPython Notes for mca i year students osmania university.docx
Python Notes for mca i year students osmania university.docx
 
Understanding Accommodations and Modifications
Understanding  Accommodations and ModificationsUnderstanding  Accommodations and Modifications
Understanding Accommodations and Modifications
 
Food safety_Challenges food safety laboratories_.pdf
Food safety_Challenges food safety laboratories_.pdfFood safety_Challenges food safety laboratories_.pdf
Food safety_Challenges food safety laboratories_.pdf
 
Accessible Digital Futures project (20/03/2024)
Accessible Digital Futures project (20/03/2024)Accessible Digital Futures project (20/03/2024)
Accessible Digital Futures project (20/03/2024)
 

Copernican revolution

  • 1. The Copernican Revolution The Beginning of Modern Astronomy
  • 2. The 15th Century • In 1453 Ottoman Turks overrun Constantinople. • Romans flee west into Europe and take books with them. • This end the Middle Ages. • Most people cannot read or write and generally believe that:
  • 3. The 15th Century Astronomy • Earth is stationary sphere at the center of heaven. It’s habitable surface is a flat circle with Jerusalem at it’s center. • Stars and planets made of a perfect substance called aether a 5th heavenly element. • Moon, sun and stars held in place by invisible crystalline spheres. • Heaven is its own sphere above the stars. • Hell is where Satan lives and is below the habitable surface of earth.
  • 4. 99 Years That Shook Astronomy
  • 5. Recall that astronomical models need to explain the following observations of the sky: 1. Why does the celestial sphere appear to move east to west each day (diurnal motion)? 2. Why do the Sun and planets appear to move eastward along the Zodiac? 3. How can planetary alignments such as oppositions and conjunctions be explained? 4. Why are Mercury and Venus never seen opposite of the Sun in the sky? 5. Why do planets have retrograde motion that causes them to appear to go backwards?
  • 7. Nicholas Copernicus (1473- 1543)Polish Catholic Cleric Observed night sky from an observation tower. Trying to solve the calendar problem. Suggested a Sun centered Universe in a book titled De Revolutionibus, which was not published until the year he died. NOTE: He was well educated and had read Greek astronomy.
  • 8. Copernican Model • Heliocentric Universe • De Revolutionibus Orbiun Celestium (On the Revolutions of the Heavenly Spheres) • Idea was opposed by the Catholic Church (recall Cosmas flat earth and pagans round earth.) http://es.rice.edu/ES/humsoc/Galileo/Images/Astro/Conceptions/copernican_universe.gif
  • 10. Copernican Model Explained • Earth’s rotation caused daily motion from east to west. • Mercury and Venus were inferior planets, which explained why they are always seen near the Sun. • Sun’s annual motion along the ecliptic (Zodiac) was caused by Earth’s orbital motion (this one was difficult to accept.) • Retrograde motion was a natural phenomenon of one planet passing another planet as they orbited the Sun.
  • 11. Retrograde Motion As a faster moving planet overtakes and passes a slower moving superior planet the superior planet appears to move backwards as you pass by it.
  • 12. Copernican Model Why believe Copernican model? • Ptolemy’s model had worked for 1500 years. • Ptolemy’s model provided a metaphor of the earth and humans living at the center of God’s creation. • Copernicus did not prove that the Earth orbited the Sun. • Copernican model did not predict the positions of planets any better than Ptolemy’s model.
  • 13. Occam’s Razor • William of Occam England, 14th Century • "If you have two theories which both explain the observed facts then you should use the simplest until more evidence comes along“ • "The simplest explanation for some phenomenon is more likely to be accurate than more complicated explanations.“ • KISS (instructor’s editorial comment)
  • 14. Copernican Model Why believe Copernican model? • It was aesthetically more pleasing. • It was more simple. • It explained complex motions as naturally occurring.
  • 15. SN 1572, Tycho's Supernova ''On the 11th day of November in the evening after sunset, I was contemplating the stars in a clear sky. I noticed that a new and unusual star, surpassing the other stars in brilliancy, was shining almost directly above my head; and since I had, from boyhood, known all the stars of the heavens perfectly, it was quite evident to me that there had never been any star in that place of the sky, even the smallest, to say nothing of a star so conspicuous and bright as this. I was so astonished of this sight that I was not ashamed to doubt the trustworthiness of my own eyes. But when I observed that others, on having the place pointed out to them, could see that there was really a star there, I had no further doubts. A miracle indeed, one that has never been previously seen before our time, in any age since the beginning of the world.'' http://www.seds.org/~spider/spider/Vars/sn1572.html
  • 17. Tycho Brahe (1546-1607) • Supernova caused him to do research astronomy • Danish nobleman • Keen eyed observer • Had a gold nose. • Built an observatory named Uraniborg on the Danish island of Hveen.
  • 18. Tycho’s Observatory • Used for 20 years. • Largest quadrants in the world. • Made the most accurate observation’s of planetary and star positions (+ 1 arcminute.) • 1 arcminute is 1/60 of a degree.
  • 19. Johannes Kepler (1571-1630) • German Lutheran theologian & mathematician. • Sought to prove Copernican model correct. • He saw the model representing God in the center of the universe with his creation surrounding him.
  • 20. Kepler’s Model • He believed that God created the universe using the language of geometry. • Used the 5 regular solids with equal sized faces to hold up the celestial spheres. • That explained why there were only 6 planets. • TOTALLY WRONG, but he believed in it until he died.
  • 21. Kepler & Tycho • Kepler was exiled from Graz for being Lutheran. • Tycho had left Uraniborg for Prague. • Tycho invited Kepler to join him Prague. • A strained relationship and collaboration developed. (They did not like each other!)
  • 22. Kepler & Tycho • Kepler needed Tycho’s precise observations to prove his model of nested spheres. • Tycho needed Kepler’s theoretical and mathematical mind to prove Tycho’s model to be correct (a strange combination of an Earth centered and Copernican model that never gained favor.)
  • 23. SN 1604, Kepler's Supernova http://www.seds.org/~spider/spider/Vars/sn1604.html http://en.wikipedia.org/wiki/Johannes_Kepler A few years before Tycho died another supernova was observed by Kepler in constellation of Ophiuchus on October 17th 1604. It had been observed by others as early as Oct. 4th . (Last known supernova in Milky Way.)
  • 24. Kepler & Tycho • After Tycho’s death, and many court battles with his relatives, Kepler gained access to Tycho’s data. • Tycho had always claimed that the data for Mars was the most difficult to reconcile with any theory. • Working on Mars caused Kepler to abandon perfect circular orbits and replace them with elliptical orbits.
  • 25. Kepler’s Laws 1st Law • Planets orbit the Sun in elliptical paths with the Sun at one focus.
  • 27. Kepler’s Laws 2nd Law • Law of Areas • A line connecting the Sun and a planet sweeps out equal areas in equal times. • This means that a planet moves fastest when it is closest to the Sun.
  • 28. Kepler’s Laws 3rd Law • The Harmonic Law • P2 = a3 where – P = orbital period in years – a = semi-major axis in Astronomical Units (au). An au = average distance between Earth and Sun ~ 93,000,000 miles or 150,000,000 Km.
  • 29. Kepler’s Laws 3rd Law • Example Calculation for Jupiter • a = 5.2 au’s • P2 = a3 substituting for a • P2 = (5.2)3 = 5.2 x 5.2 x 5.2 = 140.6 • Take square root of 140.6 • P = 11.86 years
  • 30. Review of Kepler’s Laws 1st Law 2nd Law 3rd Law
  • 31. Galileo Galilei (1564-1642) • The father of Physics • First person to point a telescope at the night sky. • In 1610 he wrote The Starry Messenger in which he published his observations.
  • 32. Galileo’s Telescopic Discoveries • Craters on Moon • Sunspots • Moon’s of Jupiter • Phases of Venus All of these data were used as evidence for the Copernican Model. Replica of Galileo’s telescope from http://www.museum.vic.gov.au/scidiscovery/scientists/galileo.asp
  • 33. Craters on the Moon • Moon is NOT perfect • It has craters • It has mountains http://www.hao.ucar.edu/public/education/sp/images/galileo.html
  • 34. Sunspots • Sun is NOT perfect. • It has dark spots. • What are sunspots? • The Sun may rotate, which implies the Earth may rotate. http://www.sunblock99.org.uk/sb99/people/KMacpher/first_obs.html
  • 35. Moons of Jupiter • January 7-15, 1610 • These moon’s do not revolve around the Earth or the Sun! • They form a miniature solar system of their own.
  • 37. Isaac Newton (1642-1727) • Develops Laws of Motion • Develops idea of gravity to get Edmund Halley off his back. • Halley paid to publish Mathematical Principles of Natural Philosophy. • Derived Kepler’s three laws of planetary motion using laws of motion and gravity. http://www.hao.ucar.edu/public/education/sp/images/newton.html
  • 38. Newton’s Laws 1st Law • Law of Inertia • A body at rest will remain at rest, and a body in motion will remain in motion, unless acted upon by an unbalanced force.
  • 39. Newton’s Laws 2nd Law • An acceleration is caused by an unbalanced force acting on an object and is directly proportional to the magnitude (strength) of the force applied in the direction of the force. • a α F
  • 40. Newton’s Laws 2nd Law • The acceleration of an object being acted upon by an unbalanced force is inversely proportional to the object’s mass, m. • a α 1/m
  • 41. Newton’s Laws 2nd Law • Force Law • F = ma • Force units are, F = (kg)(m/s2 ) = N ( 1 Newton). • 1N ~ the weight of an apple.
  • 42. Newton’s Laws 3rd Law • Action and Reaction • For every action there is an equal and opposite reaction. • F1 = -F2 • m1a1 = -m2a2 • Forces act in opposite directions on different objects.
  • 44. Gravity Every object in the universe appears to attract every other object in the universe with a force that is directly proportional to the product of their masses and inversely proportional to the square of the distances between them. • F α (m1m2)/r2 • F = G(m1m2)/r2 , where G is the gravitational constant. • G = 6.67x10-11 Nm2 /kg2
  • 45. The Gravity of the Situation A quick lesson on the Nature of Science Is it the Law of Gravity or the Theory of Gravity?
  • 46. Newton’s Laws 2nd Law Mass & Weight • Mass is not equal to weight. • Weight is force of gravity acting on a mass. • F = ma = mg. • W = mg. • W = (1.0kg)(9.8m/s2 ) = 9.8N.
  • 48. Resources Chaisson and McMillian, (2002). Astronomy Today (4th Ed.) Hewitt, (1998). Conceptual Physics (8th Ed.) http://www.usoe.k12.ut.us/curr/science/sciber00/8th/forces/s Shipman, Wilson, and Todd, (2003). An Introduction to Physical Science (10th Edition).