gravity r2,1 r2 r1 by m 2,1

Similar documents
2/24/2014. The point mass. Impulse for a single collision The impulse of a force is a vector. The Center of Mass. System of particles

Chapter 8. Linear Momentum, Impulse, and Collisions

10/15/2013. PHY 113 C General Physics I 11 AM-12:15 PM MWF Olin 101

Physics 2A Chapter 11 - Universal Gravitation Fall 2017

Physics 11b Lecture #2. Electric Field Electric Flux Gauss s Law

PHYS 1443 Section 003 Lecture #21

Physics 207 Lecture 16

Physics 202, Lecture 2. Announcements

24-2: Electric Potential Energy. 24-1: What is physics

Physics 1501 Lecture 19

PHYS Week 5. Reading Journals today from tables. WebAssign due Wed nite

Chapter 23: Electric Potential

Chapter I Matrices, Vectors, & Vector Calculus 1-1, 1-9, 1-10, 1-11, 1-17, 1-18, 1-25, 1-27, 1-36, 1-37, 1-41.

Energy in Closed Systems

3.1 Electrostatic Potential Energy and Potential Difference

Chapter Fifiteen. Surfaces Revisited

Potential Theory. Copyright 2004

CHAPTER 15 SPECIAL PERTURBATIONS

PHY126 Summer Session I, 2008

Rigid Bodies: Equivalent Systems of Forces

PHYS 705: Classical Mechanics. Derivation of Lagrange Equations from D Alembert s Principle

Chapter 13 - Universal Gravitation

7/1/2008. Adhi Harmoko S. a c = v 2 /r. F c = m x a c = m x v 2 /r. Ontang Anting Moment of Inertia. Energy

CHAPTER 3 SYSTEMS OF PARTICLES

CSJM University Class: B.Sc.-II Sub:Physics Paper-II Title: Electromagnetics Unit-1: Electrostatics Lecture: 1 to 4

Scalars and Vectors Scalar

Set of square-integrable function 2 L : function space F

iclicker Quiz a) True b) False Theoretical physics: the eternal quest for a missing minus sign and/or a factor of two. Which will be an issue today?

r ˆr F = Section 2: Newton s Law of Gravitation m 2 m 1 Consider two masses and, separated by distance Gravitational force on due to is

COLLEGE OF FOUNDATION AND GENERAL STUDIES PUTRAJAYA CAMPUS FINAL EXAMINATION TRIMESTER /2017

Escape Velocity. GMm ] B

Physics 3A: Linear Momentum. Physics 3A: Linear Momentum. Physics 3A: Linear Momentum. Physics 3A: Linear Momentum

PHYSICS OF ASTROPHSYICS - Energy

Engineering Mechanics. Force resultants, Torques, Scalar Products, Equivalent Force systems

THE EQUIVALENCE OF GRAM-SCHMIDT AND QR FACTORIZATION (page 227) Gram-Schmidt provides another way to compute a QR decomposition: n

Integral Vector Operations and Related Theorems Applications in Mechanics and E&M

LINEAR MOMENTUM. product of the mass m and the velocity v r of an object r r

Rotational Kinematics. Rigid Object about a Fixed Axis Western HS AP Physics 1

Remember: When an object falls due to gravity its potential energy decreases.

Physics Exam II Chapters 25-29

Fundamental principles

ALL QUESTIONS ARE WORTH 20 POINTS. WORK OUT FIVE PROBLEMS.

Objectives. Chapter 6. Learning Outcome. Newton's Laws in Action. Reflection: Reflection: 6.2 Gravitational Field

CHAPTER 10 ROTATIONAL MOTION

One-dimensional kinematics

PHY121 Formula Sheet

CSU ATS601 Fall Other reading: Vallis 2.1, 2.2; Marshall and Plumb Ch. 6; Holton Ch. 2; Schubert Ch r or v i = v r + r (3.

Physics Exam 3

Linear Momentum. Center of Mass.

MULTIPOLE FIELDS. Multipoles, 2 l poles. Monopoles, dipoles, quadrupoles, octupoles... Electric Dipole R 1 R 2. P(r,θ,φ) e r

A. Thicknesses and Densities

8 Baire Category Theorem and Uniform Boundedness

1. A body will remain in a state of rest, or of uniform motion in a straight line unless it

Elastic Collisions. Definition: two point masses on which no external forces act collide without losing any energy.

If there are k binding constraints at x then re-label these constraints so that they are the first k constraints.

a v2 r a' (4v) 2 16 v2 mg mg (2.4kg)(9.8m / s 2 ) 23.52N 23.52N N

PHYS 1443 Section 002 Lecture #20

Test 1 phy What mass of a material with density ρ is required to make a hollow spherical shell having inner radius r i and outer radius r o?

Dynamics of Rigid Bodies

Physics 1: Mechanics

Electric potential energy Electrostatic force does work on a particle : Potential energy (: i initial state f : final state):

Review of Vector Algebra and Vector Calculus Operations

Extra notes for circular motion: Circular motion : v keeps changing, maybe both speed and

Stellar Astrophysics. dt dr. GM r. The current model for treating convection in stellar interiors is called mixing length theory:

CHAPTER 5: Circular Motion; Gravitation

Capítulo. Three Dimensions

total If no external forces act, the total linear momentum of the system is conserved. This occurs in collisions and explosions.

UNIT10 PLANE OF REGRESSION

BALANCING OF ROTATING MASSES

PHYS 2421 Fields and Waves

Part V: Velocity and Acceleration Analysis of Mechanisms

DYNAMICS VECTOR MECHANICS FOR ENGINEERS: Kinematics of Rigid Bodies in Three Dimensions. Seventh Edition CHAPTER

Mechanics Physics 151

Chapter 8. Momentum Impulse and Collisions. Analysis of motion: 2 key ideas. Newton s laws of motion. Conservation of Energy

Physics for Scientists & Engineers 2

Class 6 - Circular Motion and Gravitation

Please initial the statement below to show that you have read it

One Dimension Again. Chapter Fourteen

Chapter 5 Force and Motion

Look over Chapter 22 sections 1-8 Examples 2, 4, 5, Look over Chapter 16 sections 7-9 examples 6, 7, 8, 9. Things To Know 1/22/2008 PHYS 2212

= 4 3 π( m) 3 (5480 kg m 3 ) = kg.

Determining solar characteristics using planetary data

Uniform Circular Motion

Physics 201 Lecture 4

OSCILLATIONS AND GRAVITATION

Consider two masses m 1 at x = x 1 and m 2 at x 2.

19 The Born-Oppenheimer Approximation

ω = θ θ o = θ θ = s r v = rω

4 SingularValue Decomposition (SVD)

LINEAR MOMENTUM Physical quantities that we have been using to characterize the motion of a particle

MAGNETISM MAGNETIC DIPOLES

Physics 114 Exam 2 Fall 2014 Solutions. Name:

2 dependence in the electrostatic force means that it is also

Chapter 5 Force and Motion

Physic 231 Lecture 14

Physics 207: Lecture 20. Today s Agenda Homework for Monday

Khintchine-Type Inequalities and Their Applications in Optimization

Chap13. Universal Gravitation

Physics 231. Topic 8: Rotational Motion. Alex Brown October MSU Physics 231 Fall

Orbital Angular Momentum Eigenfunctions

Transcription:

Gavtaton Many of the foundatons of classcal echancs wee fst dscoveed when phlosophes (ealy scentsts and atheatcans) ted to explan the oton of planets and stas. Newton s ost faous fo unfyng the oton of heavenly bodes wth those on eath (an apple). Newton s law of Unvesal Gavtaton has now been supeseded by Ensten s Geneal Relatvty, but just as eale, Newton s appoxaton s vey good n any stuatons and thus vey wothy of study. G The classcal law of gavtaton s often wtten as F ˆ gavty, whee G s a unvesal constant equal to 6.67 x 0 - N kg -, and s the sepaaton between the asses. Howeve ths s not pecse enough fo us. Consde two sphecal asses,, and the foce of gavty between the, ˆ, F on by G We want to know the foced placed on by o F,. Ths s equal to F, ˆ, whee ˆ s the unt vecto that ponts fo to. (The way to eebe the ode of the subscpts s fnal nus ntal.) The negatve sgn ndcates that the foce s attactve and puts the foce n the opposte decton fo the unt vecto. So knowng the foce placed on by, what about the convese, the foce placed on by, o F? Clealy fo the syety of the expesson these foces ae equal n agntude, but opposte n decton. (Ths s an exaple of Newton s thd laws that states that f an object places a foce on anothe, then t expeences an equal and opposte placed by the othe on t. Newton s thd law s by fa the ost coplcated of hs thee to undestand and apply coectly. An untold nube of

ntoductoy physcs students have gotten theselves ted up n knots tyng to fgue out whee to put the eacton foce. You have been foewaned! One hnt, the eacton foce s neve put on the object expeencng the ognal foce.) Takng a close look at the fgue above ases an potant queston. was defned to be the dstance between the centes of the sphecal objects. Why was ths selected; why not the suface to-suface dstance? O what happens when the object s not sphecal? The Unvesal Law of Gavtaton s well defned fo pont asses. Ths s a good appoxaton when the objects ae vey fa apat, such that the ad ae uch salle than the sepaaton. But n the fgue above that s not the case. The sepaaton s only ~0 tes the ad of the asses. Ae we akng a poo appoxaton? To exane ths poble, consde the gavtatonal attacton between a pont ass,, and an abtay extended object, M. Thee s no estcton placed on the sepaaton between the two. M How can we use the Unvesal Law of Gavtaton to detene the foce F M, that body M puts on? You ay be thnkng that you need to fnd the Cente of Mass, o CM of object M, but ths s not coect. (Although t s a thoughtful guess and the appoach to take s sla to that taken to fnd the CM.) Consde a sall poton of ass M, fo conceteness a vey sall cube soewhee wthn the body. The Unvesal Law of Gavtaton allows us to fnd the foce between the sall cube and ass. Specfcally, t s F ˆ, G, whee s the ass of the cube and s the dstance between the cube and. s now well defned because the postons of and ae pecse. Of couse, ths can be done fo a second pont

F, F, Now the net foce on the pont ass fo both and s the just the sple vecto addton of the ndvdual foces, F F F net,, Fnet fo and You can know see whee ths s gong. Consde dcng the whole of the extended object M nto lttle peces. (The shape of the lttle peces s abtay, howeve soetes the syety of the object suggests a shape.) Then the net foce on would be gven by, F G. If we know the densty () of the extended object as a functon of ˆ, M, poston then the aount of ass n each lttle pece s ( ) V and the next foce ( ) V becoes: F ˆ, M G,. Now ths s an expesson that can be used on a copute to fnd the net foce placed by M on. The copute can be pogaed to su ove a vast nube of lttle boxes usng the appopate densty, dstance and decton. Howeve, atheatcally t s vey useful to take the lt as the nube of boxes goes to nfnty. Takng ogn of the coodnate syste to be at the pont ass, the expesson becoes ( ) V ( ) F ˆ ˆ, M G l, G dv M. Ths s an ntegal ove the volue of the extended object, wth beng a vecto that ognates at the locaton of the pont ass and

tenates wthn ass M. You can agne the end of ths vecto beng oved all ove the ( ) extent of M as t s beng noalzed, ultpled by and sued up. If ths looks coplcated to you, you ae ght, t can be. You wll have a chance to do ths type of ntegal n Calc III. Fo the te beng t s enough to know n pncple how t s done and be able to do t nuecally. It s nteestng to note that because the total foce depends lnealy on the pont ass, t s often convenent to talk about the foce that would be placed on a test patcle of ass as FM, () FM, g o convesely defne gm (). Ths s the concept of a feld, n ths case the gavtatonal feld. The feld fo ass M exsts wthout the pesence of the second patcle to expeence t. One way to pctue the gavtatonal feld s a collecton of aows pontng n the decton that a test ass would acceleate f t wee placed at a locaton and havng a agntude gven by ts acceleaton. Hee s a athe poo endton

( ) ' Fo each pont n space you would need to fnd gm () G dv M ( ) ', whee the ntegal s ove the ped vaables and dv. Ths need not be easy, but t can be done, and s a vey useful concept. What s potant now s that you begn to thnk about such a gavtatonal feld as aows exstng n space aound all assve objects and that these aows tell you the acceleaton that would occu f a test ass was placed thee. We have coe a long way n ou dscusson of gavty, but have not copletely answeed ou queston about how to handle the gavtatonal attacton between extended objects. We know that n geneal the foce nvolves sung up contbutons fo all ove the objects. Consdeng the ognal stuaton, ths looks qute dffcult. We even have to su ove two objects! Thee ust be a way out, ˆ, F on by and thee s, but only n a vey specal case.