1. Earth’s Shape and Size Unit 1

2. The Earth’s Shape Earth’s shape is nearly spherical (Oblate Spheroid) It is flattened at the poles and bulging at the equator This makes a person weigh slightly more at the poles than at the equator

3. Earth’s surface is very smooth The height of Mt. Everest is only 7/10,000 of Earth’s diameter

4. Ancient Observations of Earth Shadow of Earth during an eclipse Position of the stars as travelers moved north or south A ship’s mast disappeared last as it sailed towards the horizon Aristotle, as early as the 3 rd century BC concluded that the earth was a sphere.

5. Using the North Star The North Star (Polaris) appears to increase in altitude as you travel north It is always visible due north to an observer north of the equator –90 0 for someone at the North Pole –0 0 for someone at the Equator If the earth were flat, Polaris would appear the same to everyone.

7. Today…. Photographs from space are the best way to see the shape of the earth

8. Other proof that the earth is round/spherical

9. Pre Lab Info Roundness Ratio –Tells us how close something is to a perfect circle –A perfect circle would have a roundness ration of 1 because the diameter would be the same in all directions

10. Pre Lab Info Scale Models are concrete representations of an object that is made in proportion to the object –They may be larger (ex. Model of an atom) –They may be smaller (ex. Globe)

11. Finding the Proportions Think ratio: Part to whole = Part to whole Matchbox cars are made on a ratio of 1:59 This means that the Matchbox car is 59 times smaller than the real car. Using the Matchbox car, figure out how big the real car is.

12. 1/59 = 7.1/X X = 418.9 cm How many meters is this? 4.189 m 7.1 cm