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February 10th 2012

February 10th 2012 . ESSENTIAL QUESTION:. Describe and apply Kepler’s Three Laws 2 nd Per: Describe the evolution of the Heliocentric model. LEARNING OBJECTIVE:. Understand Kepler’s Second Law and the history behind it. 2 nd : Understand how the Geocentric model evolved.

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February 10th 2012

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  1. February 10th 2012 ESSENTIAL QUESTION: Describe and apply Kepler’s Three Laws 2nd Per: Describe the evolution of the Heliocentric model LEARNING OBJECTIVE: Understand Kepler’s Second Law and the history behind it. 2nd: Understand how the Geocentric model evolved WARM UP: 1,3-6 Are the ellipses that you drew yesterday an accurate portrayal of planet’s orbits? If not, how would it need to be changed. 2nd In your activity yesterday what is declination and right ascension? Also tell me in which directions are these measured (from their respective Point zero in which direction do they move) AGENDA • Warm up • Ellipse Lab • 2nd Per- Retrograde Motion Activity and book work

  2. February 10th, 2012 FORMATIVE ASSESSMENT: . Teacher led Questions on student’s understanding of today’s lesson. VOCABULARY: heliocentric, geocentric, epicycle, retrograde, potential energy, kinetic energy, Kepler’s 3 Laws. Perihelion, Aphelion, Semi major axis, Semi-Minor Axis, declination, right ascension. . PRACTICE: ASSIGNMENTS: Book assignment – Due Retrograde Motion Assignment Due Warm ups Due NOTES:

  3. February 9th 2012 ESSENTIAL QUESTION: Describe and apply Kepler’s Three Laws 2nd Per: Describe the evolution of the Heliocentric model LEARNING OBJECTIVE: Understand Kepler’s Second Law and the history behind it. 2nd: Understand how the Geocentric model evolved WARM UP: Suppose you receive a message from aliens living on a planet orbiting a star similar to ours. They say they live 4 times further from their star than Earth is from the Sun. How does the length of their year compare to ours? Come up with a name for their year! AGENDA • Warm up • Kepler’s Laws (2nd Per – geocentric model) • Task analysis – Kepler’s Laws, • 2nd Per- Retrograde Motion Activity and book work

  4. February 9th, 2012 FORMATIVE ASSESSMENT: . Teacher led Questions on student’s understanding of today’s lesson. VOCABULARY: heliocentric, geocentric, epicycle, retrograde, potential energy, kinetic energy, Kepler’s 3 Laws. Perihelion, Aphelion . PRACTICE: ASSIGNMENTS: Book assignment – Due Retrograde Motion Assignment Due Warm ups Due NOTES:

  5. February 8th 2012 ESSENTIAL QUESTION: Describe and apply Kepler’s Three Laws 2nd Per: Describe the evolution of the Heliocentric model LEARNING OBJECTIVE: Understand Kepler’s Second Law and the history behind it. 2nd: Understand how the Geocentric model evolved WARM UP: See next Slide AGENDA • Warm up • Kepler’s Laws (2nd Per – geocentric model) • Task analysis – Kepler’s Laws, • 2nd Per- Retrograde Motion Activity and book work

  6. WARM UP: Period 1,3,4-6 There is three planet solar system (planet Beta, Delta and Gamma, planets orbiting a 2 solar mass star. Planet Gamma is 6 AU, Planet Delta is 3 AU and the last planet’s distance (Beta) is unknown but its orbital period is 0.5 Earth years long. What is planet G and D’s period, what is Planet B’s distance for its parent star? If the sun tripled its mass how would it change the periods and/or distances. BTW why is there no Alpha Planet? Period 2 What are epicycles? What did they help explain?

  7. February 8th, 2012 FORMATIVE ASSESSMENT: . Teacher led Questions on student’s understanding of today’s lesson. VOCABULARY: heliocentric, geocentric, epicycle, retrograde, potential energy, kinetic energy, Kepler’s 3 Laws. Perihelion, Aphelion . PRACTICE: ASSIGNMENTS: Book assignment – Due Retrograde Motion Assignment Due Warm ups Due NOTES:

  8. February 7th 2012 ESSENTIAL QUESTION: Describe and apply Kepler’s Three Laws 2nd Per: Describe the evolution of the Heliocentric model LEARNING OBJECTIVE: Understand Kepler’s First Laws and the history behind it. 2nd: Understand how the Geocentric model evolved WARM UP: Part 1) What do YOU think is the conservation of angular Momentum. Part 2) After watching demo what do YOU think is conservation angular momentum AGENDA • Warm up • Kepler’s Laws (2nd Per – geocentric model) • Task analysis – Kepler’s Laws, • 2nd Per- Retrograde Motion Activity and book work

  9. February 7th, 2012 FORMATIVE ASSESSMENT: . Teacher led Questions on student’s understanding of today’s lesson. VOCABULARY: heliocentric, geocentric, epicycle, retrograde, potential energy, kinetic energy, Kepler’s 3 Laws. Perihelion, Aphelion . PRACTICE: ASSIGNMENTS: Book assignment – Due Retrograde Motion Assignment Due Warm ups Due NOTES:

  10. February 6th 2012 ESSENTIAL QUESTION: Describe and apply Kepler’s Three Laws LEARNING OBJECTIVE: Understand Kepler’s First Laws and the history behind it. WARM UP: Solve for the P - And yes you better get a calculator for this chapter A3 = P2 When A = 1, A = 0.7, A = 1.5, A = 5.2. Take your answer and multply by 365. AGENDA • Warm up • Kepler’s Laws

  11. February 6th, 2012 FORMATIVE ASSESSMENT: . Teacher led Questions on student’s understanding of today’s lesson. VOCABULARY: heliocentric, geocentric, epicycle, retrograde, potential energy, kinetic energy, Kepler’s 3 Laws. Perihelion, Aphelion . PRACTICE: ASSIGNMENTS: Book assignment – Due Retrograde Motion Assignment Due Warm ups Due NOTES:

  12. February 3rd 2012 Quiz On a separate sheet of paper – short answers: What is the difference between “geocentric” and “heliocentric”? (2 pts) What are epicycles and why were they created (2pts) EXPLAIN the two major problems with the epicycle model and how were they “corrected” (the correct terms are not necessary). Bonus if you can ADD the third minor problem that the epicycle model exhibited. (4 pts) plus 1 bonus pt. What did Copernicus give us? What was the one thing it did not change from the Greek model. (2 pts)

  13. Perihelion Inferior Conjunction Aphelion Opposition Conjunction EARTH Superior Conjunction

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