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Introduction to SAT II Physics - FreeExamPapers

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10. B<br />

Kepler’s Third Law tells us that T 2 /a 3 is a constant for every planet in a system. If we let xT be the value<br />

for the period of planet B ’s orbit, then we can solve for x using a bit of algebra:<br />

Thermal <strong>Physics</strong><br />

THERMAL PHYSICS IS ESSENTIALLY THE study of heat, temperature, and heat transfer.<br />

As we shall see—particularly when we look at the Second Law of Thermodynamics—these<br />

concepts have a far broader range of application than you may at first imagine. All of these<br />

concepts are closely related <strong>to</strong> thermal energy, which is one of the most important forms of<br />

energy. In almost every energy transformation, some thermal energy is produced in the form of<br />

heat. To take an example that by now should be familiar, friction produces heat. Rub your hands<br />

briskly <strong>to</strong>gether and you’ll feel heat produced by friction.<br />

When you slide a book along a table, the book will not remain in motion, as New<strong>to</strong>n’s First Law<br />

would lead us <strong>to</strong> expect, because friction between the book and the table causes the book <strong>to</strong> slow<br />

down and s<strong>to</strong>p. As the velocity of the book decreases, so does its kinetic energy, but this decrease<br />

is not a startling violation of the law of conservation of energy. Rather, the kinetic energy of the<br />

book is slowly transformed in<strong>to</strong> thermal energy. Because friction acts over a relatively large<br />

distance, neither the table nor the book will be noticeably warmer. However, if you were somehow<br />

able <strong>to</strong> measure the heat produced through friction, you would find that the <strong>to</strong>tal heat produced in<br />

bringing the book <strong>to</strong> a s<strong>to</strong>p is equal <strong>to</strong> the book’s initial kinetic energy.<br />

Technically speaking, thermal energy is the energy associated with the random vibration and<br />

movement of molecules. All matter consists of trillions of trillions of tiny molecules, none of<br />

which are entirely still. The degree <strong>to</strong> which they move determines the amount of thermal energy<br />

in an object.<br />

While thermal energy comes in<strong>to</strong> play in a wide range of phenomena, <strong>SAT</strong> <strong>II</strong> <strong>Physics</strong> will focus<br />

primarily on the sorts of things you might associate with words like heat and temperature. We’ll<br />

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