sg14 - Chapter 14 Study Guide for Gravitation 14.1...

Info iconThis preview shows pages 1–3. Sign up to view the full content.

View Full Document Right Arrow Icon
Chapter 14 Study Guide for Gravitation 14.1 Universal gravitation Skill 14.1 Understand the role of the gravitational force in maintaining the orbital motion of the planets. Don’t get rotational velocity and orbital velocity confused. Rotational velocity is the velocity of rotation of an object about an axis through its center. Orbital velocity is the tangential velocity of an object orbiting another object. In the absence of external forces, all planets would follow straight-line trajectories. The fact that they move in approximately circular paths means that there must be a centripetal force acting on them. As Newton Frst postulated, the centripetal force that holds the planets in their orbits is the gravitational force. Skill 14.2 Understand the fundamental properties of the gravitational force. A solid sphere exerts a gravitational force as if all the matter in the sphere were concentrated at its center. ±urthermore, this gravitational force drops o² as 1 r 2 (the larger the distance between the interacting objects, the weaker the gravitational attraction). By equating gravitational acceleration to centripetal acceleration, we Fnd that the square of the period of a planetary orbit is proportional to the cube of the orbit’s radius (Kepler’s Third Law): 1 R 2 a g = a c v 2 R = p 2 πR T P 2 1 R R 2 T 2 . (14.1) = T 2 R 3 (14.2) The gravitational force exerted by the earth on an object is proportional to the object’s gravitational mass , which is equivalent to the object’s inertia. Similarly, the gravitational force exerted by an object on the earth is proportional to the earth’s gravitational mass. By putting together all of this information, we are able to arrive at Newton’s law of universal gravitation : F g 12 m 1 m 2 r 2 . (14.3) Note: Newton’s law of universal gravitation applies to all the gravitational mass in the universe. 1
Background image of page 1

Info iconThis preview has intentionally blurred sections. Sign up to view the full version.

View Full Document Right Arrow Icon
14.2 Gravitation and angular momentum Skill 14.3 Understand how information about the orbital motion of planets is obtained from the fact that gravitation is a central force. Gravitation is a type of central force - a force whose line of action always lies along the line connecting the two interacting objects. The central force is directed to a point called the force center . The torque caused by any central force about the force center is always zero . This is because the central force always lies along the radius vector from the force center. As a result, any object subject to a central force has a constant angular momentum about the force center (remember, change in angular momentum is due to a net external torque). The angular momentum of any particle about the origin is proportional to the rate at which area is swept out by the particle’s position vector (Look at Figure 14.9). Since angular momentum is constant for planetary orbits, the above rate must also be constant. This is stated
Background image of page 2
Image of page 3
This is the end of the preview. Sign up to access the rest of the document.

{[ snackBarMessage ]}

Page1 / 6

sg14 - Chapter 14 Study Guide for Gravitation 14.1...

This preview shows document pages 1 - 3. Sign up to view the full document.

View Full Document Right Arrow Icon
Ask a homework question - tutors are online