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5) d- L= Conclusions: 1) Which ellipse is the most circular? 2) Which ellipse is the most eccentric? 3) Describe what happens to an ellipse's eccentricity as the focal distance increases. 4) Using your ESRT which ellipse has an eccentricity closest to that of Mercury? 6) Because Earth has an elliptical orbit what happens to the apparent size of the Sun throughout the year? 7) A-What is the Eccentricity of Earth? B- Is ellipse #1(on the front page) :More, Less or The Same (circle one) as the orbit of Earth? C- Write a sentence supporting your answer to 7B (use numerical data to support your answer) 4) 3) Procedure: KEPLER'S ELLIPSES 1) Using your ESRT or a ruler measure the focal distance for the ellipse. 2) Using your ESRT or a ruler measure the major axis length for the ellipse. 3) Calculate the eccentricity for the ellipse. (SHOW ALL WORK) 4) Repeat this procedure for each ellipse shown. Ellipses: 1) d= L= 0.217317 2) d = L= e= d = €5 -0.023 小小 L= e= d = L=

5) d- L= Conclusions: 1) Which ellipse is the most circular? 2) Which ellipse is the most eccentric? 3) Describe what happens to an ellipse's eccentricity as the focal distance increases. 4) Using your ESRT which ellipse has an eccentricity closest to that of Mercury? 6) Because Earth has an elliptical orbit what happens to the apparent size of the Sun throughout the year? 7) A-What is the Eccentricity of Earth? B- Is ellipse #1(on the front page) :More, Less or The Same (circle one) as the orbit of Earth? C- Write a sentence supporting your answer to 7B (use numerical data to support your answer) 4) 3) Procedure: KEPLER'S ELLIPSES 1) Using your ESRT or a ruler measure the focal distance for the ellipse. 2) Using your ESRT or a ruler measure the major axis length for the ellipse. 3) Calculate the eccentricity for the ellipse. (SHOW ALL WORK) 4) Repeat this procedure for each ellipse shown. Ellipses: 1) d= L= 0.217317 2) d = L= e= d = €5 -0.023 小小 L= e= d = L=

Applications and Investigations in Earth Science (9th Edition)
Applications and Investigations in Earth Science (9th Edition)
9th Edition
ISBN:9780134746241
Author:Edward J. Tarbuck, Frederick K. Lutgens, Dennis G. Tasa
Publisher:Edward J. Tarbuck, Frederick K. Lutgens, Dennis G. Tasa
Chapter1: The Study Of Minerals
Section: Chapter Questions
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5) d- L= Conclusions: 1) Which ellipse is the most circular? 2) Which ellipse is the most eccentric? 3) Describe what happens to an ellipse's eccentricity as the focal distance increases. 4) Using your ESRT which ellipse has an eccentricity closest to that of Mercury? 6) Because Earth has an elliptical orbit what happens to the apparent size of the Sun throughout the year? 7) A-What is the Eccentricity of Earth? B- Is ellipse #1(on the front page) :More, Less or The Same (circle one) as the orbit of Earth? C- Write a sentence supporting your answer to 7B (use numerical data to support your answer)
Transcribed Image Text:5) d- L= Conclusions: 1) Which ellipse is the most circular? 2) Which ellipse is the most eccentric? 3) Describe what happens to an ellipse's eccentricity as the focal distance increases. 4) Using your ESRT which ellipse has an eccentricity closest to that of Mercury? 6) Because Earth has an elliptical orbit what happens to the apparent size of the Sun throughout the year? 7) A-What is the Eccentricity of Earth? B- Is ellipse #1(on the front page) :More, Less or The Same (circle one) as the orbit of Earth? C- Write a sentence supporting your answer to 7B (use numerical data to support your answer)
4) 3) Procedure: KEPLER'S ELLIPSES 1) Using your ESRT or a ruler measure the focal distance for the ellipse. 2) Using your ESRT or a ruler measure the major axis length for the ellipse. 3) Calculate the eccentricity for the ellipse. (SHOW ALL WORK) 4) Repeat this procedure for each ellipse shown. Ellipses: 1) d= L= 0.217317 2) d = L= e= d = €5 -0.023 小小 L= e= d = L=
Transcribed Image Text:4) 3) Procedure: KEPLER'S ELLIPSES 1) Using your ESRT or a ruler measure the focal distance for the ellipse. 2) Using your ESRT or a ruler measure the major axis length for the ellipse. 3) Calculate the eccentricity for the ellipse. (SHOW ALL WORK) 4) Repeat this procedure for each ellipse shown. Ellipses: 1) d= L= 0.217317 2) d = L= e= d = €5 -0.023 小小 L= e= d = L=
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