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Chapter 14 Resource: Plate Tectonics
Chapter 14 Resource: Plate Tectonics

Sample Unit of Study - New York Science Teacher
Sample Unit of Study - New York Science Teacher

... 1. The Earth is made of several different materials arranged in layers by density. 2. Heat generated motions in these layers controls the shape and structure of the surface. 3. The surface is divided into a number of rigid plates that move against each other creating the surface features. 4. Earthqu ...
1 - hrsbstaff.ednet.ns.ca
1 - hrsbstaff.ednet.ns.ca

... 52. In an effort to create a cannonball-style splash, eight-year old Matthew runs off the edge of the board of the high dive at 4.6 m/s and falls 2.3 m to the water below. a. Determine the time for Matthew to fall the 2.3 m to the water. (0.685s) b. What horizontal distance from the edge of the boar ...
Review of the Earth Science Curriculum FROM McGUIRE Equations
Review of the Earth Science Curriculum FROM McGUIRE Equations

... *The moon’s period of rotation and revolution are equal, so the same side of the moon always faces Earth *Half of the moon is always lit *Moon’s orbit is tilted at an angle of about 5 degrees with respect to Earth’s orbit *Seasonal variations in temperatures result from parallelism, the tilt of Eart ...
Venus atmosphere and climate
Venus atmosphere and climate

... – Venus and Earth are assumed to have formed from essentially the same material, with the same initial amounts of H2O, CO2, N2, etc... – But divergent evolution occurred because: • Venus is closer to the Sun, so H2O can exist only in vapor (gas) form. • At Earth's distance, liquid H2O could form. ...
Chapter 7 Earth: Our Home in Space
Chapter 7 Earth: Our Home in Space

... –where M is Earth’s mass and Mm is the Moon’s mass. •Assuming that the mass of the Moon is far less than the mass of the Earth, ...
Lesson 2
Lesson 2

Downloadable Structure PP
Downloadable Structure PP

... - the inner core is a solid (it’s hotter than the outer core, but the high pressure makes it solid - from 5100 km depth to: ≈ 6354 km at the poles ≈ 6378 km at the equator * spin of the earth results in an equitorial bulge ...
Ch1-Earth_s Layers - Mater Academy Lakes High School
Ch1-Earth_s Layers - Mater Academy Lakes High School

... • Earth’s major landforms include plains, plateaus, and mountains. Plains have low relief and low elevation. Plateaus have low relief and high elevation. Mountains have high relief and high elevation. ...
Ch 3_sec1 Class notes
Ch 3_sec1 Class notes

... • Over the past 15 million to 20 million years, large numbers of earthquakes have occurred along the San Andreas Fault in California, where parts of the North America plate and the Pacific plate are slipping past one another. ...
Chapter 2
Chapter 2

Plate Tectonics
Plate Tectonics

Earth Science Mid Term 2007 Part 1
Earth Science Mid Term 2007 Part 1

... locations, A, B, C, and D. Movement of the crustal sections (plates) is indicated by arrows, and the locations of frequent earthquakes are indicated by an asterisk. Diagrams are not drawn to scale. Which location best represents the boundary between the African plate and the South ...
Plate Tectonics
Plate Tectonics

... Mountains in North America bear a striking resemblance to the Caledonian Mountains in Europe (e.g., similar age of rocks) • Although thousands of kilometres apart, the two mountain ranges must have been formed by the same geologic forces ...
Elasticity and Anisotropy of Common Crustal Minerals
Elasticity and Anisotropy of Common Crustal Minerals

Earth Works - LSU AgCenter
Earth Works - LSU AgCenter

Layers of the Earth
Layers of the Earth

Chapter 2 - Dublin City Schools
Chapter 2 - Dublin City Schools

earthquake ppt
earthquake ppt

... HOW DO TECTONIC PLATES CAUSE EARTHQUAKES? ...
Earthquake Unit Assessment Retake Preparation
Earthquake Unit Assessment Retake Preparation

Unit 1
Unit 1

... 9. Spectroscopic studies of the sun have been made over many years and many data have been accumulated. 10. For those who live on the equator, days and nights will always be equal. 11. The known history of the earth has been more or less definitely divided into great eras, and these, in turn, into p ...
2001310 Earth Space Science Study Guide
2001310 Earth Space Science Study Guide

... Explain  how  hurricanes  form  in  relation  to  latitude. Define  carbon  neutrality. Be  able  to  identify  the  relationship  of  relative  humidity  to  weather conditions. Explain  possible  preventative  methods  for  reducing  rip  current ...
Plate Tectonics OmniGlobe Lesson Plan Grade / Class / Subject
Plate Tectonics OmniGlobe Lesson Plan Grade / Class / Subject

... Many of the objects scientist study, like planets or atoms, are too big or too small to work with by hand. Too sole this problem, scientists build scale model, like shrinking a planet down to the size of a basketball or blowing an atom up to the size of a baseball. Scale models make objects easier f ...
Chapter 1: ​ Matter in Motion ppt
Chapter 1: ​ Matter in Motion ppt

...  Why doesn’t the sun’s gravitational force affect you more than Earth’s does? It is because it is so far away.  If you could stand on the sun, you would find it impossible to move. The gravitational force on you would be so strong that you could not move. ...
Lesson 7 - Plate Tectonics, Earthquakes and Volcanoes
Lesson 7 - Plate Tectonics, Earthquakes and Volcanoes

... plants (in the form of coal deposits) in Antarctica led to the conclusion that this frozen land previously must have been situated closer to the equator, in a more temperate climate where lush, swampy vegetation could grow; distinctive fossil ferns (Glossopteris) discovered in now-polar regions; gla ...
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Schiehallion experiment



The Schiehallion experiment was an 18th-century experiment to determine the mean density of the Earth. Funded by a grant from the Royal Society, it was conducted in the summer of 1774 around the Scottish mountain of Schiehallion, Perthshire. The experiment involved measuring the tiny deflection of a pendulum due to the gravitational attraction of a nearby mountain. Schiehallion was considered the ideal location after a search for candidate mountains, thanks to its isolation and almost symmetrical shape. One of the triggers for the experiment were anomalies noted during the survey of the Mason–Dixon Line.The experiment had previously been considered, but rejected, by Isaac Newton as a practical demonstration of his theory of gravitation. However, a team of scientists, notably Nevil Maskelyne, the Astronomer Royal, were convinced that the effect would be detectable and undertook to conduct the experiment. The deflection angle depended on the relative densities and volumes of the Earth and the mountain: if the density and volume of Schiehallion could be ascertained, then so could the density of the Earth. Once this was known, then this would in turn yield approximate values for those of the other planets, their moons, and the Sun, previously known only in terms of their relative ratios. As an additional benefit, the concept of contour lines, devised to simplify the process of surveying the mountain, later became a standard technique in cartography.
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