1. The diameter of the Sun is 1,391,400 km. The diameter of the Moon is 3,474.8 km. Find the ratio, r= DSun/DMoon between the sizes. r= [Dsun/ Dmaan) r= [1,391,400 / 3,474.8] r= 400.425 r= 400.425 2. From the point of view of an observer on Earth (consider the Earth as a point-like object), during the eclipse, the Moon covers the Sun exactly. Sketch a picture to illustrate this fact. Use a ruler to get a straight line. Your drawing does not need to be in scale. 3. The Sun is 1 Astronomical Unit (AU) away from the Earth. Find the distance between the Earth and the Moon in AU's using the ratio of similar triangles. Show your work. DE/M =. Convert this to kilometers. Use 1 AU=149,600,000 km. AU. DE/M=, km.
1. The diameter of the Sun is 1,391,400 km. The diameter of the Moon is 3,474.8 km. Find the ratio, r= DSun/DMoon between the sizes. r= [Dsun/ Dmaan) r= [1,391,400 / 3,474.8] r= 400.425 r= 400.425 2. From the point of view of an observer on Earth (consider the Earth as a point-like object), during the eclipse, the Moon covers the Sun exactly. Sketch a picture to illustrate this fact. Use a ruler to get a straight line. Your drawing does not need to be in scale. 3. The Sun is 1 Astronomical Unit (AU) away from the Earth. Find the distance between the Earth and the Moon in AU's using the ratio of similar triangles. Show your work. DE/M =. Convert this to kilometers. Use 1 AU=149,600,000 km. AU. DE/M=, km.
Principles of Physics: A Calculus-Based Text
5th Edition
ISBN:9781133104261
Author:Raymond A. Serway, John W. Jewett
Publisher:Raymond A. Serway, John W. Jewett
Chapter1: Introduction And Vectors
Section: Chapter Questions
Problem 56P: The distance from the Sun to the nearest star is about 4 1016 m. The Milky Way galaxy (Fig. P1.56)...
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