1 CHAPTER 10 ROCKET MOTION

Similar documents
Lecture L14 - Variable Mass Systems: The Rocket Equation

G U I D E T O A P P L I E D O R B I T A L M E C H A N I C S F O R K E R B A L S P A C E P R O G R A M

Fluid Mechanics Prof. S. K. Som Department of Mechanical Engineering Indian Institute of Technology, Kharagpur

GRAVITATIONAL FIELDS PHYSICS 20 GRAVITATIONAL FORCES. Gravitational Fields (or Acceleration Due to Gravity) Symbol: Definition: Units:

SPEED, VELOCITY, AND ACCELERATION

1 of 7 9/5/2009 6:12 PM

A = 6561 times greater. B. 81 times greater. C. equally strong. D. 1/81 as great. E. (1/81) 2 = 1/6561 as great.

Use the following information to deduce that the gravitational field strength at the surface of the Earth is approximately 10 N kg 1.

2. Orbits. FER-Zagreb, Satellite communication systems 2011/12

How Rockets Work Newton s Laws of Motion

F = ma. F = G m 1m 2 R 2

Forces on the Rocket. Rocket Dynamics. Equation of Motion: F = Ma

Lab #4 - Linear Impulse and Momentum

Lecture L17 - Orbit Transfers and Interplanetary Trajectories

Mechanics 1: Conservation of Energy and Momentum

Newton s Law of Universal Gravitation

Name: Earth 110 Exploration of the Solar System Assignment 1: Celestial Motions and Forces Due in class Tuesday, Jan. 20, 2015

Physics 41 HW Set 1 Chapter 15

circular motion & gravitation physics 111N

Work and Energy. Work = Force Distance. Work increases the energy of an object. Energy can be converted back to work.

Lecture L22-2D Rigid Body Dynamics: Work and Energy

Mathematical Modeling and Engineering Problem Solving

Section 4: The Basics of Satellite Orbits

v v ax v a x a v a v = = = Since F = ma, it follows that a = F/m. The mass of the arrow is unchanged, and ( )

Motion of a Leaky Tank Car

Name Class Period. F = G m 1 m 2 d 2. G =6.67 x Nm 2 /kg 2

LINEAR EQUATIONS IN TWO VARIABLES

Numerical Solution of Differential Equations

1 Speed of light is the maximal possible speed

Halliday, Resnick & Walker Chapter 13. Gravitation. Physics 1A PHYS1121 Professor Michael Burton

1. Fluids Mechanics and Fluid Properties. 1.1 Objectives of this section. 1.2 Fluids

This means there are two equilibrium solutions 0 and K. dx = rx(1 x). x(1 x) dt = r

Newton s Laws. Newton s Imaginary Cannon. Michael Fowler Physics 142E Lec 6 Jan 22, 2009

Chapter 15 Collision Theory

Review D: Potential Energy and the Conservation of Mechanical Energy

Some Special Relativity Formulas

Force. Force as a Vector Real Forces versus Convenience The System Mass Newton s Second Law. Outline

Can Hubble be Moved to the International Space Station? 1

PHYS 101 Lecture 10 - Work and kinetic energy 10-1

Chapter 7 Momentum and Impulse

Forces. When an object is pushed or pulled, we say that a force is exerted on it.

To define concepts such as distance, displacement, speed, velocity, and acceleration.

Magnetism. d. gives the direction of the force on a charge moving in a magnetic field. b. results in negative charges moving. clockwise.

A MONTE CARLO DISPERSION ANALYSIS OF A ROCKET FLIGHT SIMULATION SOFTWARE

Lecture-IV. Contact forces & Newton s laws of motion

ACTIVITY 6: Falling Objects

Solving Systems of Two Equations Algebraically

HEAT UNIT 1.1 KINETIC THEORY OF GASES Introduction Postulates of Kinetic Theory of Gases

Lecture L2 - Degrees of Freedom and Constraints, Rectilinear Motion

Newton s Laws of Motion

8. As a cart travels around a horizontal circular track, the cart must undergo a change in (1) velocity (3) speed (2) inertia (4) weight

Halliday, Resnick & Walker Chapter 13. Gravitation. Physics 1A PHYS1121 Professor Michael Burton

Version A Page The diagram shows two bowling balls, A and B, each having a mass of 7.00 kilograms, placed 2.00 meters apart.

SIMPLIFIED METHOD FOR ESTIMATING THE FLIGHT PERFORMANCE OF A HOBBY ROCKET

Satellites and Space Stations

Review Vocabulary force: a push or a pull. Vocabulary Newton s third law of motion

Stability Analysis of Small Satellite Formation Flying and Reconfiguration Missions in Deep Space

Introduction to Netlogo: A Newton s Law of Gravity Simulation

Uniformly Accelerated Motion

Chapter 3 Falling Objects and Projectile Motion

Physics Kinematics Model

AP PHYSICS C Mechanics - SUMMER ASSIGNMENT FOR

PS-6.2 Explain the factors that determine potential and kinetic energy and the transformation of one to the other.

Displacement (x) Velocity (v) Acceleration (a) x = f(t) differentiate v = dx Acceleration Velocity (v) Displacement x

3 Work, Power and Energy

Physical Science Chapter 2. Forces

Niraj Sir GRAVITATION CONCEPTS. Kepler's law of planetry motion

Practice Test SHM with Answers

Prelab Exercises: Hooke's Law and the Behavior of Springs

JET ENGINE PERFORMANCE. Charles Robert O Neill. School of Mechanical and Aerospace Engineering. Oklahoma State University. Stillwater, OK 74078

Chapter 4 One Dimensional Kinematics

CHAPTER 6 WORK AND ENERGY

Differential Relations for Fluid Flow. Acceleration field of a fluid. The differential equation of mass conservation

Speed, velocity and acceleration

General Physical Science

DIRECT ORBITAL DYNAMICS: USING INDEPENDENT ORBITAL TERMS TO TREAT BODIES AS ORBITING EACH OTHER DIRECTLY WHILE IN MOTION

Applications of Second-Order Differential Equations

Does currently available technology have the capacity to facilitate a manned mission to Mars?

Physics 40 Lab 1: Tests of Newton s Second Law

Ion Propulsion Engine Simulation

Newton s Laws Quiz Review

Chapter 6. Work and Energy

Section 6.4: Work. We illustrate with an example.

Figure 1. Diode circuit model

Eðlisfræði 2, vor 2007

Exam Three Momentum Concept Questions

Chapter 8 Conservation of Linear Momentum. Conservation of Linear Momentum

physics 111N work & energy

Gravitational Potential Energy

Wind Turbine Power Calculations

Notes: Most of the material in this chapter is taken from Young and Freedman, Chap. 13.

2 ONE- DIMENSIONAL MOTION

Chapter 4: Newton s Laws: Explaining Motion

Physics Notes Class 11 CHAPTER 6 WORK, ENERGY AND POWER

Physics: Principles and Applications, 6e Giancoli Chapter 4 Dynamics: Newton's Laws of Motion

9. Momentum and Collisions in One Dimension*

Interaction of Energy and Matter Gravity Measurement: Using Doppler Shifts to Measure Mass Concentration TEACHER GUIDE

x 1 ' = x 1 vt 1 x 1 ' = 4.0 m t 1 = 1.0 s x 2 vt 2 ' = 4.0 m t 2 ' = x 2 = 3.0 s x 1 = x 2 x 1 ' + vt 1 ' + vt 2 v (t 1 t 2 ) = x 2 ' x 1 ' = x 2

Unit 4 Practice Test: Rotational Motion

Transcription:

1 CHAPTER 1 ROCKET MOTION 1. Introduction If you are asked to state Newton's Second Law of Motion, I hope you will not reply: "Force equals mass times acceleration" because that is not Newton's Second Law of Motion. Newton's Second Law of Motion is: The alteration of motion is ever proportional to the motive force impressed; and is made in the direction of the right line in which that force is impressed. In short: Force equals Rate of Change of Momentum, or, in symbols, F = p&. On differentiating the right hand side, we obtain F = mv& + mv &. In other words, if the mass is constant then indeed force equals mass times acceleration but only if the mass is constant. In a rocket, a very appreciable fraction of the mass of the rocket is fuel, which is burned and ejected at a very high rate, so that the mass of the rocket is rapidly diminishing during the motion. It is one of the great problems of rocket design that such a high proportion of the initial mass must be fuel. For this reason, other possible methods of driving spacecraft are being investigated by many groups. For example, in the ion propulsion system of the Deep Space One spacecraft, electrically accelerated ions are ejected at high speed from the spacecraft. The force produced and the acceleration are minute, but, because it can be kept up for a very long time, very high speeds can eventually be reached. "Solar sail" systems similarly rely on the very tiny force that can be exerted by the solar wind, but this tiny force can be exerted during most of the lifetime of a spacecraft's flight, and hence again high speeds can be reached. This chapter, however, concerns just conventional rocket motion. In the next section I consider the motion of a rocket in space subject only to the one force from the high-speed ejection of burned fuel in the absence of any other forces. At a later date, if I can find the time and energy, I may add further sections on rocket motion against gravity, which might be uniform or might fall off with distance from Earth, and we might include air resistance or not. But to begin with, we deal solely with a rocket isolated in space and subject to no additional forces. 2. An Integral So that we don't get bogged down later with an integral that is going to crop up, see if you can do the following integration: ( a bt) ln. You should get t ( a bt) ln( a bt)+ 1 b constant.

2 3. The Rocket Equation. Initially at time t =, the mass of the rocket, including fuel, is m. We suppose that the rocket is burning fuel at a rate of b kg s -1 so that, at time t, the mass of the rocket-plus-remaining-fuel is m = m bt. The rate of increase of mass with time is dm = b and is supposed constant with time. (The rate of "increase" is, of course, negative.) We suppose that the speed of the ejected fuel, relative to the rocket, is V. The thrust of the ejected fuel on the rocket is therefore Vb, or V dm. This is equal to the instantaneous mass times acceleration of the rocket: Vb dv dv = m = ( m ). bt 1.3.1 v t Thus. dv = Vb 1.3.2 m bt t (Don't be tempted to write the right hand side as Vb. You are anticipating a bt m logarithm, so keep the denominator positive. We have met this before in Chapter 6.) On integration, we obtain v = V ln m. m bt 1.3.3 The acceleration is dv = Vb. 1.3.4 m bt At t =, the speed is zero and the acceleration is Vb/m. At time t = m /b, the remaining mass is zero and the speed and acceleration are both infinite. However, this is so only if the initial mass is 1% fuel and nothing else. This is not realistic. If the fraction of the total mass was initially f, the fuel will be completely expended after a time fm /b at which time the speed will be V ln ( 1 f ) (which is, of course, positive), and the speed will remain constant thereafter. For example, if f = 99%, the final speed will be 4.6V.

3 Equations 1.3.3 and 1.3.4 are shown in figures X.1 and X.2. In figure X.1, the speed of the rocket is plotted in units of V, the ejection speed of the burnt fuel. The time is plotted in units of m /b. The fuel initially comprised 9% of the rocket, so that the rocket runs out of fuel in time.9 m /b, at which time its speed is 2.3V. In figure X.2, the acceleration is plotted in units of the initial acceleration, which is Vb/m. When the fuel is exhausted, the acceleration is ten times this.

4 In equation 1.3.3, v is of course dx/, so the equation can be integrated to obtain the distance:time relation: m bt x = V t + t ln 1. 1.3.5 b m Elimination of t between equations 1.3.3 and 1.3.5 gives the relation between speed and distance: x Vm v 1 1 + e V = v / V b. 1.3.6 If f is the fraction of the initial mass that is fuel, the fuel supply will be exhausted after a time fm /b, at which time its speed will be V ln( 1 f ), (this is positive, because 1 f is less than 1), its acceleration will be 1/(1 f) and it will have travelled a distance Vm [ f + ( 1 f ) ln( 1 f )]. If the entire initial mass is fuel, so that f = 1, the fuel will burn b for a time m i /b, at which time its speed and acceleration will be infinite, it will have travelled a finite distance Vm /b and the mass will have been reduced to zero, This remarkable result is not very believable, for two reasons. In the first place it is not very realistic. More importantly, when the speed becomes comparable to the speed of light, the equations which we have developed for nonrelativistic speeds are no longer approximately valid, and the correct relativistic equations must be used. The speed cannot then reach the speed of light as long as the remaining mass is non-zero. Equations 1.3.5 and 1.3.6 are illustrated in figures X.3 and X.4, in which f, the fraction of the initial mass that is fuel, is.9. The units for distance, time and speed in these graphs are, respectively, Vm /b, m /b and V.

5

6 4. Problems (i) Derive the integral in section 2. (ii) Integrate equation 1.3.2 to obtain equation 1.3.3 (iii) Integrate equation 1.3.3 to obtain equation 1.3.5 (iv) Obtain equation 1.3.6 In the following problems, (numbers v - viii) assume V = 2 km s -1. m = 2 kg b =.5 kg s -1 f = 9% (v) What is the maximum speed, and how long does it take to attain it? (vi) How long does it take to reach a speed of 3 km s -1? (vii) How long does it take for the rocket to travel 6 km? (viii) How fast is it moving when it has travelled 3 km?