chapt01-Introduction理论力学第一章英文课件.ppt
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1、 2004 The McGraw-Hill Companies, Inc. All rights reserved. 1 - 11.1. What is Mechanics? The science which describes and predicts the conditions of rest or motion of bodies under the action of forces1. Mechanics of rigid bodies (GE 204, 205)2. Mechanics of deformable bodies (GE 206)3. Mechanics of fl
2、uids (CE, ME 308) 2004 The McGraw-Hill Companies, Inc. All rights reserved. 1 - 2Mechanics Statics (dealing with bodies at rest) and Dynamics (bodies in motion) Assumed to be perfectly rigid for statics and dynamics Fluid mechanics; compressible and incompressible flow (hydraulic, or low velocity ae
3、rodynamics) Mechanics uses mathematics, but applied science for engineering applications 2004 The McGraw-Hill Companies, Inc. All rights reserved. 1 - 31.2 Fundamental Concepts and Principles Study of Mechanics goes back to Aristotle (384-322 B.C.) and Archimedes (287-212 B.C.) Isaac Newton (1642-17
4、27) DAlembert, Lagrange and Hamilton Einstein; theory of relativity (1905) 2004 The McGraw-Hill Companies, Inc. All rights reserved. 1 - 4Aristotle Fourth century B.C.E. Mechanical Problems; collections of questions and answers; in physics, mathematics and engineering Among 35 mechanical problems po
5、sed by Aristotle Why are larger balancesmore accurate than smaller ones? Why are pieces of timber weaker the longer they are, and why do they bend more easily when raised? 2004 The McGraw-Hill Companies, Inc. All rights reserved. 1 - 5 Renaissance shipbuilders found that their large timber ships wer
6、e breaking under their own weight Galileo (1638) prefaced his seminal study of strength of material by reciting the breakup of ships, etc. Still there are failures of heavy steel ships and large missiles Factor of safety or factor of ignorance? 2004 The McGraw-Hill Companies, Inc. All rights reserve
7、d. 1 - 6Galileos seminal work on strength of materials and dynamicsDialogues Concerning Two New Sciences 2004 The McGraw-Hill Companies, Inc. All rights reserved. 1 - 7Galileos illustration of two failure modesMarble lying on the ground can be soiled, discolored and hard to lift again.Inclined again
8、st wall can cause crack or it may fall.Best way is put on the support. 2004 The McGraw-Hill Companies, Inc. All rights reserved. 1 - 8 2004 The McGraw-Hill Companies, Inc. All rights reserved. 1 - 9Failed Liberty ship, c.1940 2004 The McGraw-Hill Companies, Inc. All rights reserved. 1 - 10 2004 The
9、McGraw-Hill Companies, Inc. All rights reserved. 1 - 11WSGalileos PostulationLSbhWhbhSWL222 2004 The McGraw-Hill Companies, Inc. All rights reserved. 1 - 12Galileo, 1638hbXWLShbXLSbhWbbhSXL2 ,2222 2004 The McGraw-Hill Companies, Inc. All rights reserved. 1 - 13Correcting the Error Can you tell what
10、is wrong? 17th century Hookes law 1729 Bernard Forest de Balidor following the earlier lead of Leibniz and P. Varignon found that LSbhWhbhSWL332 2004 The McGraw-Hill Companies, Inc. All rights reserved. 1 - 14WSForests PostulationLSbhWhbhSWL332 2004 The McGraw-Hill Companies, Inc. All rights reserve
11、d. 1 - 15Edme Mariottes experiments; while designing pipelines to supply water to the palace at Versailles 2004 The McGraw-Hill Companies, Inc. All rights reserved. 1 - 16 Marriotte recognized that there must be linearly varying compression as well as tension acting across the beams section He had e
12、rror in calculating resultant moment, and he used Galileos formula 1713, A. Parent found correct treatment but was ignored because Was not pubished by French Academy Many misprints and poorly edited He was not a clear writer He criticized many others work 2004 The McGraw-Hill Companies, Inc. All rig
13、hts reserved. 1 - 171.2 Continued Basic concepts used in mechanics; space, time, mass and force Space; position of the point P; coordinates of P with reference to the origin In Newtonian mechanics; space, time, and mass are absolute concepts, independent each other (force is not independent) Note; r
14、elativistic mechanics time is not independent 2004 The McGraw-Hill Companies, Inc. All rights reserved. 1 - 181.2 Continued Force is a vector; point of application, magnitude and direction Study the conditions of rest or motion of particles and rigid bodies in terms of the four basic concepts Partic
15、les; a very small amount of matter which may be assumed to occupy a single point in space Rigid bodies; a combination of a large number of particles occupying fixed positions with respect to each other 2004 The McGraw-Hill Companies, Inc. All rights reserved. 1 - 19Six Fundamental Principles All pri
16、nciples are based on experimental evidence, not from mathematical derivations1. Parallelogram law for addition of Forces The two forces acting on a particle may be replaced by a single force; resultant Parallelogram Law 2004 The McGraw-Hill Companies, Inc. All rights reserved. 1 - 202. The Principle
17、 of TransmissibilityThe conditions of equilibrium or of motion of a rigid body will remain unchanged if a force acting at a given point of the rigid body is replaced by a force of the same magnitude and same direction, but acting at a different pointFFThe same line of actionSee Chapter 3 2004 The Mc
18、Graw-Hill Companies, Inc. All rights reserved. 1 - 213. Newtons First Law; if the resultant force acting on a particle is zero, the particle will remain at rest (if originally at rest) or will move with constant speed in a straight line (if originally in motion)TDLW 2004 The McGraw-Hill Companies, I
19、nc. All rights reserved. 1 - 224. Newtons Second Law If the resultant force acting on a particle is not zero, the particle will have an acceleration proportional to the magintude of the resultant and in the direction of this resultant force F=ma5. Newtons Third Law The force of action and reaction b
20、etween bodies in contact have the same magnitude, same line of action, and opposite senseSee Chapter 6 2004 The McGraw-Hill Companies, Inc. All rights reserved. Photo 1.1 2004 The McGraw-Hill Companies, Inc. All rights reserved. 1 - 246. The Newtons Law of Gravitation2rMmGF 2RMGg R; radius of the ea
21、rthW=mgg; 9.81 m/s2 or 32.2 ft/s2 2004 The McGraw-Hill Companies, Inc. All rights reserved. 1 - 25Units and Dimensions; Objectives Know the difference between units and dimensions Understand the SI, USCS (U.S. Customary System, or British Gravitational System), and AES (American Engineering) systems
22、 of units Know the SI prefixes from nano- to giga- Understand and apply the concept of dimensional homogeneity 2004 The McGraw-Hill Companies, Inc. All rights reserved. 1 - 26Objectives What is the difference between an absolute and a gravitational system of units? What is a coherent system of units
23、? Apply dimensional homogeneity to constants and equations. 2004 The McGraw-Hill Companies, Inc. All rights reserved. 1 - 27Introduction France in 1840 legislated official adoption of the metric system and made its use be mandatory In U.S., in 1866, the metric system was made legal, but its use was
24、not compulsory 2004 The McGraw-Hill Companies, Inc. All rights reserved. 1 - 28Measurement StandardzInch, foot; based on human bodyz4000 B.C. Egypt; Kings Elbow=0.4633 m, 1.5 ft, 2 handspans, 6 hand-widths, 24 finger-thicknesszAD 1101 King Henry I yard (0.9144 m) from his nose to the tip of his thum
25、bz1528 French physician J. Fernel distance between Paris and Amiens 2004 The McGraw-Hill Companies, Inc. All rights reserved. 1 - 29Measurement Standardz1872, Meter (in Greek, metron to measure)- 1/10 of a millionth of the distance between the North Pole and the equatorzPlatinum (90%)-iridium (10%)
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