This document provides instructions for navigating a presentation on circular motion and gravitation. It begins with directions for viewing the presentation as a slideshow and advancing through it. It then lists the chapter's content sections and objectives. The remainder of the document consists of slides from the presentation covering topics like centripetal acceleration, force, Kepler's laws of planetary motion, and torque.
36. Sample Problem, continued Chapter 7 Use Table 1 in the textbook to find the values for the radius ( r 2 ) and mass ( m ) of Venus. r 2 = 6.05 10 6 m m = 4.87 10 24 kg Find r by adding the distance between the spacecraft and Venus’s surface ( r 1 ) to Venus’s radius ( r 2 ). r = r 1 + r 2 r = 3.61 10 5 m + 6.05 10 6 m = 6.41 10 6 m Section 3 Motion in Space
37. Sample Problem, continued Chapter 7 3. Calculate 4. Evaluate Magellan takes (5.66 10 3 s)(1 min/60 s) 94 min to complete one orbit. Section 3 Motion in Space
45. Torque and the Lever Arm Chapter 7 Section 4 Torque and Simple Machines In each example, the cat is pushing on the door at the same distance from the axis. To produce the same torque, the cat must apply greater force for smaller angles.
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47. The Sign of a Torque Chapter 7 Section 4 Torque and Simple Machines