قراءة كتاب Common Science

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Common Science

Common Science

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دار النشر: Project Gutenberg
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subjects rather than according to daily lessons. The varying lengths of recitation periods in different schools, and the adaptation of the course to individual instruction as well as to class work, also made a division into lessons impracticable. Each teacher will soon discover about how much matter her class, if she uses the class method, can take each day. Probably the average section will require about 2 days to cover; the longest sections, 5 days. The entire course should easily be covered in one year with recitations of about 25 minutes daily. Two 50-minute periods a week give a better division of time and also ought to finish the course in a year. Under the individual system, the slowest diligent children finish in 7 or 8 school months, working 4 half-hours weekly. The fastest do it in about one third that time.

Upon receipt of 20 cents, the publishers will send a manual prepared by the author, containing full instructions as to the organization and equipment of the laboratory or demonstration desk, complete lists of apparatus and material needed, and directions for the construction of a chemical laboratory.

The latter is a laboratory course in which the children are turned loose among all sorts of interesting materials and apparatus,—kaleidoscope, microscope, electric bell, toy motor, chemicals that effervesce or change color when put together, soft glass tubing to mold and blow, etc. The teacher demonstrates various experiments from time to time to show the children what can be done with these things, but the children are left free to investigate to their heart's content. There is no teaching in this introductory course other than brief answers to questions. The astronomy and geology reading usually accompany the work in introductory science.

ACKNOWLEDGMENTS

To Frederic Burk, president of the San Francisco State Normal School, I am most under obligation in connection with the preparation of this book. His ideas inspired it, and his dynamic criticism did much toward shaping it. My wife, Heluiz Chandler Washburne, gave invaluable help throughout the work, especially in the present revision of the course. One of my co-workers on the Normal School faculty, Miss Louise Mohr, rendered much assistance in the classification and selection of inferences. Miss Beatrice Harper assisted in the preparation of the tables of supplies and apparatus, published in the manual to accompany this book. And I wish to thank the children of the Normal School for their patience and cooperation in posing for the photographs. The photographs are by Joseph Marron.

CONTENTS

CHAPTER PAGE
1. Gravitation 1
1. A real place where things weigh nothing and where there is no up or down 1
2. "Water seeks its own level" 6
3. The sea of compressed air in which we live: Air pressure 10
4. Sinking and floating: Displacement 23
5. How things are kept from toppling over: Stability 29
2. Molecular Attraction 36
6. How liquids are absorbed: Capillary attraction 36
7. How things stick to one another: Adhesion 41
8. The force that makes a thing hold together: Cohesion 44
9. Friction 49
3. Conservation of Energy 57
10. Levers 57
11. Inertia 66
12. Centrifugal force 72
13. Action and reaction 77
14. Elasticity 82
4. Heat 88
15. Heat makes things expand 88
16. Cooling from expansion 94
17. Freezing and melting

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