CHAPTER ONE
Physical Quantities, Units, Dimensions, Space and Time
1.1 Introduction to Physical Measurement
Physics is concerned with the description and explanation of natural phenomena in terms of measurable quantities and mathematical relationships. Mechanics, which forms the main subject of this course, studies the motion of bodies and the forces and interactions associated with that motion.
Before motion, force, energy, momentum or gravitation can be studied quantitatively, there must be a clear understanding of measurement. A statement such as “the table is long” is qualitative. A statement such as “the table is 1.50 m long” is quantitative because a numerical value has been compared with an accepted standard called a unit.
Measurement is the process of comparing a physical quantity with an accepted standard of the same kind in order to assign a numerical value and a unit to that quantity.
A measured physical quantity therefore normally contains two essential components: a numerical magnitude and a unit. Writing a measurement without its appropriate unit can make a physical statement incomplete or meaningless.
If the length of a room is written as 8, the statement is incomplete. If it is written as 8 m, the number 8 gives the magnitude while the metre specifies the standard unit used.
1.2 Physical Quantities
A physical quantity is a measurable property of a body, substance, phenomenon or physical system that can be expressed by a numerical value together with an appropriate unit.
Length, mass, time, temperature, velocity, acceleration, force, momentum and energy are examples of physical quantities. Physics expresses relationships among such quantities using equations.
For example, the average speed of an object is related to distance and elapsed time by
Thus, physical laws are not merely collections of numbers. They describe relationships among measurable quantities.
1.3 Fundamental and Derived Quantities
Physical quantities are commonly classified as fundamental quantities and derived quantities.
Fundamental Quantities:
A fundamental or base quantity is a physical quantity chosen as independent and not defined in terms of other quantities within a given system of measurement.
The International System of Units, abbreviated SI, uses seven base quantities.
| Base Quantity | SI Base Unit | Unit Symbol |
|---|---|---|
| Length | metre | m |
| Mass | kilogram | kg |
| Time | second | s |
| Electric current | ampere | A |
| Thermodynamic temperature | kelvin | K |
| Amount of substance | mole | mol |
| Luminous intensity | candela | cd |
For mechanics, the three most frequently used base quantities are length, mass and time.
Derived Quantities:
A derived quantity is a physical quantity defined through an algebraic combination of fundamental quantities or other derived quantities.
For example, velocity is obtained from displacement divided by time, while force is obtained from mass multiplied by acceleration.
| Derived Quantity | Relation | SI Unit |
|---|---|---|
| Area | length × length | m2 |
| Volume | length × length × length | m3 |
| Velocity | displacement / time | m s-1 |
| Acceleration | velocity / time | m s-2 |
| Force | mass × acceleration | newton (N) |
| Momentum | mass × velocity | kg m s-1 |
| Work/Energy | force × displacement | joule (J) |
| Power | work / time | watt (W) |
Question: Determine the SI unit of acceleration from its definition.
Given: Acceleration is change in velocity per unit time.
Formula:
Solution:
The SI unit of velocity is
Therefore,
Answer: The SI unit of acceleration is m s-2.
Question: Deduce the SI unit of force from the relation F=ma.
Formula:
Where: m is mass and a is acceleration.
Solution:
This derived unit is called the newton.
Answer: The SI unit of force is the newton (N).
1.4 Systems of Units and the SI System
A system of units is a consistent collection of standard units used for measuring physical quantities. Historically, several systems have been used, including the centimetre-gram-second (CGS) system and the metre-kilogram-second (MKS) system.
Modern scientific work predominantly uses the International System of Units (SI). The SI provides internationally agreed standards and reduces ambiguity when measurements are communicated.
Unit symbols are not normally pluralized and are not followed by a full stop unless they occur at the end of a sentence. Thus, 5 kg, 20 m and 15 s are standard forms.
1.5 SI Prefixes and Scientific Notation
Very large and very small measurements are easier to express using powers of ten and SI prefixes.
| Prefix | Symbol | Factor |
|---|---|---|
| tera | T | 1012 |
| giga | G | 109 |
| mega | M | 106 |
| kilo | k | 103 |
| centi | c | 10-2 |
| milli | m | 10-3 |
| micro | μ | 10-6 |
| nano | n | 10-9 |
| pico | p | 10-12 |
Question: Express 7.5 km in metres.
Given:
Solution:
Answer: 7500 m.
Question: Express 0.0000042 m in micrometres.
Given:
Solution:
Therefore,
Answer: 4.2 μm.
1.6 Conversion of Units
Unit conversion changes the unit in which a quantity is expressed without changing the physical quantity itself. A reliable method is to multiply by conversion factors equal to one.
Question: Convert 72 km/h to m/s.
Given:
Solution:
Answer: 20 m/s.
Question: Convert 25 m/s to km/h.
Solution:
Answer: 90 km/h.
Question: Convert 250 cm2 to square metres.
Solution:
Since
then
Therefore,
Answer: 0.025 m2.
1.7 Dimensions and Dimensional Formulae
Units tell us the standards used to measure quantities, while dimensions describe the physical nature of quantities in terms of fundamental quantities.
In mechanics, the symbols commonly used for the fundamental dimensions are:
The dimensions of a physical quantity show how that quantity depends on fundamental quantities such as mass, length and time.
For example, velocity is length divided by time. Therefore,
Acceleration is velocity divided by time, giving
| Quantity | Relation | Dimensions |
|---|---|---|
| Area | length × length | L2 |
| Volume | length3 | L3 |
| Velocity | displacement/time | LT-1 |
| Acceleration | velocity/time | LT-2 |
| Momentum | mass × velocity | MLT-1 |
| Force | mass × acceleration | MLT-2 |
| Work/Energy | force × distance | ML2T-2 |
| Power | work/time | ML2T-3 |
1.8 Determination of Dimensions of Physical Quantities
Question: Determine the dimensions of force.
Formula:
Solution:
and
Therefore,
Answer: The dimensions of force are MLT-2.
Question: Determine the dimensions of kinetic energy.
Formula:
Solution:
The numerical constant 1/2 has no dimensions. Therefore,
Answer: [K]=ML2T-2.
Question: Pressure is defined as force per unit area. Determine its dimensions.
Formula:
Solution:
Hence,
Answer: The dimensions of pressure are ML-1T-2.
1.9 Principle of Dimensional Homogeneity
Every term in a physically meaningful equation that is added to or subtracted from another term must have the same dimensions.
Consider the equation of uniformly accelerated motion
The left-hand side has dimensions
For the first term on the right,
For the second term,
All terms have the dimension of length. The equation is therefore dimensionally homogeneous.
Question: Test whether the equation
is dimensionally consistent.
Solution:
Also,
Hence,
Answer: The equation is dimensionally consistent.
Question: Determine whether
can represent a physically valid equation for velocity.
Solution:
However,
The dimensions LT-1 and L cannot be added in a physically meaningful equation.
Answer: The equation is not dimensionally consistent.
1.10 Applications of Dimensional Analysis
Dimensional analysis is useful for checking equations, deriving the possible form of relationships and converting between systems of units.
Checking Physical Equations:
If the dimensions of the two sides of an equation are different, the equation must be incorrect. Dimensional agreement, however, does not prove that an equation is completely correct.
Determining the Form of a Relationship:
Suppose the period T of a simple pendulum is assumed to depend on its length l and gravitational acceleration g. Assume
where k is dimensionless and a and b are to be determined.
Question: Use dimensional analysis to determine how the period of a simple pendulum depends on its length l and gravitational acceleration g.
Given:
Dimensions:
Solution:
Equating powers of L:
Equating powers of T:
Therefore,
Hence,
Thus,
Answer: Dimensional analysis predicts that T is proportional to √(l/g). It cannot determine the dimensionless constant k; for a simple pendulum undergoing small oscillations, further analysis gives k=2π.
1.11 Limitations of Dimensional Analysis
Dimensional analysis is powerful, but its conclusions have limits. In particular, it cannot generally:
- determine dimensionless numerical constants such as 2, 1/2 or 2π;
- determine whether terms should be added or subtracted;
- distinguish between different physical quantities that have the same dimensions;
- derive relationships involving functions such as sine, cosine, exponential or logarithmic functions from dimensions alone;
- prove that a dimensionally correct equation is physically correct.
Work and torque both have dimensions ML2T-2, but they are physically different quantities. Dimensional equality does not imply physical equivalence.
1.12 Space, Position and Reference Frames
Mechanics describes where objects are and how their positions change. To specify position meaningfully, a reference system must be chosen.
A reference frame is a coordinate system together with a means of measuring time, relative to which the position and motion of an object are described.
In one-dimensional motion, a single coordinate such as x may be sufficient. In two dimensions, position may require coordinates (x,y), while three-dimensional motion generally requires (x,y,z).
The position of an object has meaning only relative to a chosen origin and coordinate axes. A passenger sitting inside a moving vehicle may be at rest relative to the vehicle but moving relative to an observer standing beside the road.
This dependence on a reference frame becomes especially important in the study of relative motion and Newton's laws.
1.13 Time and Time Intervals
Time provides the ordering of events and allows changes in physical systems to be described. In mechanics, the SI unit of time is the second.
A distinction should be made between a particular instant and an elapsed time interval. If an event begins at time t1 and ends at t2, the elapsed time is
Question: A motion begins at t=2.5 s and ends at t=11.8 s. Determine the elapsed time.
Formula:
Solution:
Answer: The elapsed time is 9.3 s.
1.14 Measurement, Accuracy and Precision
No experimental measurement is infinitely exact. Every measuring instrument has a finite resolution, and measurements are affected by experimental limitations. Consequently, numerical results in physics should be reported with appropriate care.
Accuracy describes how close a measured value is to the accepted or true value of the quantity.
Precision describes the degree of agreement among repeated measurements or the fineness with which a measurement is reported.
A set of measurements may be precise without being accurate. For example, an incorrectly calibrated instrument may repeatedly produce nearly identical readings that are all displaced from the accepted value.
Absolute and Percentage Error:
If xm is a measured value and xa is an accepted value, the absolute error is
The percentage error is
Question: An experimental measurement of gravitational acceleration gives 9.70 m/s2, while the accepted value for the comparison is 9.81 m/s2. Calculate the absolute and percentage errors.
Solution:
Percentage error:
Answer: Absolute error = 0.11 m/s2; percentage error ≈ 1.12%.
Chapter Summary
- Physics describes natural phenomena using measurable physical quantities and mathematical relationships.
- A physical measurement consists of a numerical magnitude and an appropriate unit.
- Physical quantities may be fundamental or derived.
- The SI has seven base quantities, with length, mass and time being especially important in mechanics.
- Derived units are obtained by combining base units according to the defining relationships of physical quantities.
- SI prefixes provide convenient ways of expressing very large and very small quantities.
- Unit conversions must account correctly for powers when area and volume units are involved.
- Dimensions express the physical nature of a quantity in terms of fundamental dimensions.
- Velocity has dimensions LT-1, acceleration LT-2 and force MLT-2.
- The principle of dimensional homogeneity requires terms that are added or equated to have compatible dimensions.
- Dimensional analysis can test equations and determine the possible form of some physical relationships.
- Dimensional analysis cannot generally determine dimensionless numerical constants.
- Position and motion are described relative to a reference frame.
- Elapsed time is the difference between final and initial times.
- Accuracy concerns closeness to an accepted value, whereas precision concerns consistency or fineness of measurement.
CHAPTER TWO
Scalars, Vectors and Vector Operations
2.1 Introduction to Scalars and Vectors
Physical quantities differ not only in their units and dimensions but also in the information required to describe them completely. Some quantities are completely specified by magnitude alone. Others require both magnitude and direction.
This distinction gives rise to two major classes of physical quantities: scalars and vectors. A sound understanding of vectors is essential in mechanics because displacement, velocity, acceleration, force, momentum, torque and angular momentum involve direction.
2.2 Scalar Quantities
A scalar is a physical quantity that is completely specified by magnitude and an appropriate unit, without the need to specify a direction.
Examples of scalar quantities include mass, time, temperature, distance, speed, energy, work, power, density and volume.
A statement that a vehicle travels at 20 m/s describes its speed. No direction is required. Speed is therefore a scalar quantity.
2.3 Vector Quantities
A vector is a physical quantity having both magnitude and direction and obeying the mathematical rules of vector addition.
Examples include displacement, velocity, acceleration, force, momentum, torque and angular momentum.
A velocity of 20 m/s east contains both magnitude and direction. If the direction changes while the magnitude remains 20 m/s, the velocity has changed even though the speed has not.
| Scalar Quantity | Corresponding Vector Quantity |
|---|---|
| Distance | Displacement |
| Speed | Velocity |
| Mass | Momentum involves mass and vector velocity |
| Energy | Force |
| Work | Torque |
2.4 Representation and Equality of Vectors
A vector is commonly represented by a directed line segment or by a bold symbol such as A. Its magnitude may be written as |A| or simply A where the context is clear.
The length of a vector arrow represents its magnitude according to an appropriate scale, while the arrowhead indicates direction.
Equal Vectors:
Two vectors are equal if they have the same magnitude and the same direction, irrespective of where they are drawn.
Negative Vector:
The negative of A, written -A, has the same magnitude as A but points in the opposite direction.
Zero Vector:
A zero vector has zero magnitude. It may arise, for example, when an object returns to its original position and consequently has zero resultant displacement.
2.5 Addition of Vectors
Vectors cannot generally be added by simply adding their magnitudes. Their directions must be taken into account.
Triangle Method:
To add vectors A and B, place the tail of B at the head of A. The resultant extends from the tail of A to the head of B.
Parallelogram Method:
If two vectors start from a common point and form adjacent sides of a parallelogram, the diagonal drawn from their common origin represents their resultant.
Question: A person walks 6 m east and then 8 m north. Determine the magnitude and direction of the resultant displacement.
Given:
Required: Resultant displacement.
Solution:
The two displacements are perpendicular. Therefore,
Let θ be the angle north of east.
Answer: The resultant displacement is 10 m at approximately 53.1° north of east.
Resultant of Two Vectors at an Arbitrary Angle:
If vectors of magnitudes A and B have an angle θ between them, the magnitude of their resultant is
Question: Two forces of magnitudes 10 N and 6 N act at an angle of 60°. Find the magnitude of their resultant.
Formula:
Solution:
Since cos60°=1/2,
Answer: The resultant force has magnitude 14 N.
2.6 Subtraction of Vectors
Subtracting a vector is equivalent to adding its negative. Therefore,
This principle is important when calculating changes in vector quantities. For example, a change in velocity is
Question: An object initially moves east at 12 m/s and later moves east at 20 m/s. Determine its change in velocity.
Solution:
Taking east as positive,
Answer: The change in velocity is 8 m/s east.
2.7 Resolution of Vectors into Components
A vector can be replaced by components along chosen coordinate directions. This process is called resolution of a vector.
For a vector A of magnitude A making an angle θ with the positive x-axis,
and
The signs of the components depend on the quadrant in which the vector lies.
Question: A force of 50 N acts at 30° above the horizontal. Determine its horizontal and vertical components.
Given:
Formula:
Solution:
Answer: Horizontal component ≈ 43.3 N; vertical component = 25 N.
Question: A displacement of 20 m is directed 40° north of east. Find its components.
Solution:
Answer: Eastward component ≈ 15.32 m; northward component ≈ 12.86 m.
2.8 Unit Vectors and Cartesian Vector Notation
A unit vector has magnitude one and is used primarily to specify direction. In Cartesian coordinates, the standard unit vectors are
directed along the positive x-, y- and z-axes respectively.
A three-dimensional vector can therefore be written as
Its magnitude is
Question: Find the magnitude of
Solution:
Answer: |A|=5.
Question: Given
and
find A+B.
Solution:
Add corresponding components:
Answer:
2.9 Magnitude and Direction from Components
If a two-dimensional vector has components Ax and Ay, its magnitude is
When the quadrant is taken into account, its direction may be obtained from
Question: A force has components
Determine its magnitude and direction.
Solution:
For the direction,
Answer: The force has magnitude 13 N and is directed approximately 22.6° above the positive x-axis.
2.10 Scalar Product of Vectors
The scalar or dot product of two vectors A and B is defined by
where θ is the angle between the vectors. The result is a scalar.
In Cartesian form,
If two non-zero vectors are perpendicular, θ=90° and
Question: Given
and
calculate A·B.
Solution:
Answer: A·B=5.
Question: Two vectors have magnitudes 6 and 8 and an angle of 60° between them. Find their scalar product.
Formula:
Solution:
Answer: The scalar product is 24.
2.11 Vector Product of Vectors
The vector or cross product of vectors A and B is a vector defined by
where n is a unit vector perpendicular to the plane containing A and B. Its direction is determined by the right-hand rule.
The magnitude is
Parallel vectors have zero cross product because sin0°=0, while perpendicular vectors produce a cross-product magnitude equal to the product of their magnitudes.
The standard unit-vector products include
Reversing the order changes the sign:
Question: Two vectors have magnitudes 5 and 4 and are perpendicular. Find the magnitude of their vector product.
Formula:
Solution:
Answer: The magnitude of the vector product is 20.
Question: Given
and
find A×B.
Solution:
Using distributivity,
Since
we obtain
Answer: A×B=-2k.
2.12 Applications of Vector Products in Mechanics
The scalar and vector products occur naturally in mechanics.
Work as a Scalar Product:
If a constant force F produces displacement s, the work done is
The result is a scalar.
Question: A force of 20 N acts through a displacement of 5 m at an angle of 60° to the displacement. Find the work done.
Formula:
Solution:
Answer: The work done is 50 J.
Torque as a Vector Product:
The torque produced by a force is expressed as
with magnitude
Here r is the position vector from the axis or pivot to the point at which the force acts.
Question: A force of 30 N is applied perpendicular to a spanner at a distance of 0.25 m from the pivot. Calculate the magnitude of the torque.
Given:
Formula:
Solution:
Answer: The torque magnitude is 7.5 N m.
2.13 Position and Displacement Vectors
The location of a particle relative to an origin can be described using a position vector. In three-dimensional Cartesian coordinates,
If a particle moves from position r1 to position r2, its displacement vector is
Question: A particle moves from
to
Determine its displacement vector and the magnitude of the displacement.
Solution:
The magnitude is
Answer: Displacement vector = 5i-4j m; magnitude ≈ 6.40 m.
2.14 Differentiation of Vectors
A vector may vary continuously with another variable such as time. If
and the Cartesian unit vectors are fixed, the derivative is obtained by differentiating each component:
Question: Given
find dA/dt.
Solution:
Differentiate each component:
and
Therefore,
Answer:
Derivative of a Scalar Multiple:
If φ(t) is a scalar function and A(t) a vector function, then
Derivative of a Dot Product:
Derivative of a Cross Product:
These rules become important when studying momentum, torque and angular momentum.
2.15 Velocity and Acceleration from Vector Functions
Vector differentiation provides a compact description of motion in two or three dimensions.
If the position vector of a particle is
its instantaneous velocity is
Its acceleration is
Question: The position vector of a particle is
Determine its velocity and acceleration at time t.
Required: v(t) and a(t).
Formula:
Solution:
Differentiate the position vector:
Differentiate again:
Answer:
Question: For the particle in Worked Example 17, find its velocity, speed and acceleration at t=2 s.
Solution:
Velocity:
The speed is the magnitude of the velocity:
Acceleration:
Answer: At t=2 s, the velocity is 8i+8j m/s, the speed is approximately 11.31 m/s, and the acceleration is 4i+12j m/s2.
Position, velocity and acceleration are linked by vector differentiation. Position tells where the particle is, velocity tells how its position is changing, and acceleration tells how its velocity is changing. This relationship provides the mathematical foundation for the study of kinematics in the next chapter.
Chapter Summary
- A scalar quantity has magnitude but does not require direction, while a vector quantity has both magnitude and direction.
- Distance, speed, mass, time and energy are scalars; displacement, velocity, acceleration, force and momentum are vectors.
- Vectors can be represented by directed line segments or by their Cartesian components.
- Vector addition may be performed geometrically or by adding corresponding components.
- Vector subtraction is equivalent to addition of the negative vector.
- A vector of magnitude A at angle θ to the positive x-axis has components Acosθ and Asinθ.
- The unit vectors i, j and k specify the positive Cartesian coordinate directions.
- The scalar product is A·B=ABcosθ and produces a scalar.
- The vector product has magnitude ABsinθ and produces a vector perpendicular to the plane of the original vectors.
- Work is an important application of the scalar product, while torque is an important application of the vector product.
- The displacement vector is the difference between final and initial position vectors.
- A vector function can be differentiated by differentiating its Cartesian components.
- Velocity is the time derivative of the position vector.
- Acceleration is the time derivative of velocity and the second time derivative of position.
- Vector methods provide the mathematical language required for the systematic study of motion and forces in mechanics.
CHAPTER THREE
Kinematics and Equations of Motion
3.1 Introduction to Kinematics
Mechanics is concerned with the motion of bodies and the causes of that motion. One major branch of mechanics, called kinematics, describes motion without first considering the forces responsible for it. Kinematics answers questions such as: Where is an object? How fast is it moving? In what direction is it moving? How rapidly is its velocity changing?
Kinematics is the branch of mechanics that describes the motion of objects in terms of quantities such as position, displacement, velocity and acceleration without considering the forces causing the motion.
To describe motion quantitatively, a reference frame and a coordinate system must first be chosen. In one-dimensional motion, an object may move along the x-axis. A positive direction is chosen, and motion in the opposite direction is treated as negative.
3.2 Position, Distance and Displacement
Position:
The position of a particle identifies its location relative to a chosen origin. In one dimension, the position may be represented by the coordinate x.
Distance:
Distance is the total length of the actual path travelled by an object. It is a scalar quantity and is always non-negative.
Displacement:
Displacement is the change in position of an object from its initial position to its final position. It is a vector quantity.
In one dimension,
where xi is the initial position and xf is the final position.
Question: A student walks 12 m east and then 5 m west. Find the total distance travelled and the displacement.
Given: First motion = 12 m east; second motion = 5 m west.
Solution:
Total distance is the sum of the path lengths:
Taking east as positive, the displacement is
Answer: Distance travelled = 17 m; displacement = 7 m east.
Distance depends on the actual route followed. Displacement depends only on the initial and final positions. An object can travel a considerable distance and still have zero displacement if it returns to its starting point.
3.3 Speed and Velocity
Speed:
Speed is the rate at which distance is travelled.
Speed is a scalar quantity. Its SI unit is metre per second, m/s.
Velocity:
Velocity is the rate of change of displacement with time. It is a vector quantity.
Question: A car travels 120 km east in 2 h. Find its average speed and average velocity.
Solution:
Since the displacement is 120 km east,
Answer: Average speed = 60 km/h; average velocity = 60 km/h east.
Question: A runner completes one full lap of a circular track of length 400 m in 50 s. Find the average speed and average velocity.
Solution:
After one complete lap, the runner returns to the starting point, so the displacement is zero.
Answer: Average speed = 8 m/s; average velocity = 0 m/s.
3.4 Average and Instantaneous Velocity
Average velocity describes motion over a finite time interval. If a particle moves from position x(t) to x(t+Δt), then
Instantaneous velocity describes the velocity at a particular instant. It is obtained by taking the limit as the time interval approaches zero:
Question: The position of a particle is given by
metres. Find its instantaneous velocity at t=4 s.
Formula:
Solution:
At t=4,
Answer: The instantaneous velocity is 26 m/s.
3.5 Acceleration
Acceleration is the rate of change of velocity with time.
Average acceleration is
Instantaneous acceleration is
Since v=dx/dt,
The SI unit of acceleration is m/s2.
Question: The velocity of a particle changes from 10 m/s to 28 m/s in 6 s. Find its average acceleration.
Formula:
Solution:
Answer: The average acceleration is 3 m/s2.
Question: The position of a particle is
Find its velocity and acceleration at t=2 s.
Solution:
Velocity:
At t=2,
Acceleration:
At t=2,
Answer: Velocity = 8 m/s; acceleration = 14 m/s2.
3.6 Motion with Constant Velocity
If a particle moves with constant velocity, its acceleration is zero. For constant velocity v,
Therefore,
If the particle begins at position x0, then its position after time t is
Question: A train moves at a constant velocity of 25 m/s for 3 minutes. Find the distance travelled.
Given:
Formula:
Solution:
Answer: The train travels 4500 m or 4.5 km.
3.7 Uniformly Accelerated Motion
A body undergoes uniform acceleration when its velocity changes by equal amounts in equal intervals of time.
For motion in a straight line with constant acceleration, the principal variables are:
| Symbol | Meaning | SI Unit |
|---|---|---|
| u | Initial velocity | m/s |
| v | Final velocity | m/s |
| a | Constant acceleration | m/s2 |
| t | Elapsed time | s |
| s | Displacement | m |
3.8 Derivation of the Equations of Motion
First Equation:
From the definition of acceleration,
Multiplying through by t,
Therefore,
Second Equation:
For constant acceleration, the average velocity is
Since displacement equals average velocity multiplied by time,
Substitute v=u+at:
Hence,
Third Equation:
From
we obtain
Using
substitute for t:
Since
then
Therefore,
Fourth Useful Form:
The displacement may also be written as
These equations are valid only when acceleration is constant during the interval under consideration.
3.9 Application of the Equations of Motion
Question: A car starts from rest and accelerates uniformly at 4 m/s2 for 6 s. Find its final velocity.
Given:
Required: Final velocity v.
Formula:
Solution:
Answer: 24 m/s.
Question: A body with initial velocity 5 m/s accelerates uniformly at 3 m/s2 for 4 s. Find its displacement.
Given:
Formula:
Solution:
Answer: The displacement is 44 m.
Question: A motorcycle moving at 20 m/s accelerates uniformly at 2.5 m/s2 over a distance of 60 m. Find its final speed.
Given:
Formula:
Solution:
Answer: The final speed is approximately 26.46 m/s.
Question: A vehicle travelling at 30 m/s is brought to rest uniformly in 5 s. Find its acceleration and stopping distance.
Given:
Acceleration:
The negative sign indicates acceleration opposite to the chosen positive direction.
Stopping Distance:
Answer: Acceleration = -6 m/s2; stopping distance = 75 m.
3.10 Graphical Description of Motion
Graphs provide a useful way to understand motion. The three most common kinematics graphs are position-time, velocity-time and acceleration-time graphs.
Position-Time Graph:
The slope of a position-time graph gives velocity:
A straight line indicates constant velocity. A curved position-time graph indicates changing velocity.
Velocity-Time Graph:
The slope of a velocity-time graph gives acceleration:
The area under a velocity-time graph gives displacement:
Acceleration-Time Graph:
The area under an acceleration-time graph gives the change in velocity:
Question: A body's velocity increases uniformly from 4 m/s to 16 m/s in 6 s. Use the velocity-time interpretation to find the acceleration and displacement.
Acceleration:
Displacement:
The area under the velocity-time graph is a trapezium:
Answer: Acceleration = 2 m/s2; displacement = 60 m.
3.11 Motion in Two Dimensions
Motion is not restricted to straight lines. A particle moving in a plane may have independent components of motion along the x- and y-directions.
The position vector can be written as
Velocity is
and acceleration is
The horizontal and vertical components can be analysed separately and then combined.
3.12 Projectile Motion
A projectile is an object that, after being launched, moves under the influence of gravity alone when air resistance is neglected.
Near the Earth's surface, the gravitational acceleration is approximately constant and directed vertically downward:
The essential feature of projectile motion is that the horizontal and vertical components of motion are independent. Neglecting air resistance:
- horizontal acceleration is zero;
- horizontal velocity remains constant;
- vertical acceleration is -g if upward is taken as positive.
3.13 Horizontal Projection
Suppose an object is projected horizontally with speed u from a height h.
Horizontal motion:
Vertical motion, if the initial vertical velocity is zero:
Question: A ball is projected horizontally at 10 m/s from the top of a cliff 20 m high. Neglect air resistance and take g=9.8 m/s2. Find the time to reach the ground and the horizontal distance travelled.
Vertical Motion:
Horizontal Motion:
Answer: Time of flight ≈ 2.02 s; horizontal distance ≈ 20.2 m.
3.14 Projection at an Angle
Suppose a projectile is launched with initial speed u at an angle θ above the horizontal. Its initial velocity components are
and
For a projectile that lands at the same vertical level from which it was launched, the standard results are:
Time of Flight:
Maximum Height:
Horizontal Range:
These formulas apply when launch and landing levels are the same and air resistance is neglected.
Question: A projectile is launched at 20 m/s at an angle of 30° above the horizontal. Take g=9.8 m/s2. Find its time of flight, maximum height and horizontal range.
Given:
Time of Flight:
Maximum Height:
Range:
Answer: Time of flight ≈ 2.04 s; maximum height ≈ 5.10 m; range ≈ 35.35 m.
Question: At what angle should a projectile be launched to obtain maximum range when it lands at its launch level?
Formula:
Solution:
For fixed u and g, range is maximum when sin2θ has its maximum value, which is 1.
Therefore,
Answer: The maximum range occurs at a launch angle of 45°.
3.15 Relative Motion
Velocity is measured relative to a reference frame. When two objects are moving, the velocity of one as observed from the other is called relative velocity.
The velocity of object A relative to object B is
Question: Car A moves east at 25 m/s and Car B moves east at 15 m/s. Find the velocity of A relative to B.
Solution:
Answer: Car A moves at 10 m/s east relative to Car B.
Question: Two cars approach each other on a straight road. Car A moves east at 20 m/s, while Car B moves west at 15 m/s. Find the velocity of A relative to B.
Solution:
Take east as positive:
Answer: The magnitude of the relative velocity is 35 m/s.
Kinematics tells us how motion occurs. It does not explain why velocity changes. To understand why an object accelerates, slows down, changes direction or remains at rest, we must introduce force and Newton's laws of motion.
Chapter Summary
- Kinematics describes motion without considering its causes.
- Distance is the total path length, while displacement is the change in position.
- Speed is a scalar rate of distance travelled, whereas velocity is a vector rate of displacement.
- Instantaneous velocity is dx/dt.
- Acceleration is the rate of change of velocity and may be written as dv/dt or d2x/dt2.
- For constant velocity, displacement is proportional to time.
- For constant acceleration, the principal equations are v=u+at, s=ut+(1/2)at2, v2=u2+2as and s=(u+v)t/2.
- The slope of a position-time graph gives velocity.
- The slope of a velocity-time graph gives acceleration, while its area gives displacement.
- The area under an acceleration-time graph gives change in velocity.
- Two-dimensional motion may be analysed by resolving it into independent Cartesian components.
- Projectile motion combines constant horizontal velocity with constant downward acceleration due to gravity.
- For equal launch and landing levels, projectile time of flight, maximum height and range can be determined from standard equations.
- The maximum horizontal range of an ideal projectile occurs at 45°.
- Relative velocity is obtained by subtracting one object's velocity vector from another's.
CHAPTER FOUR
Newton's Laws of Motion and Applications
4.1 Introduction to Dynamics
Kinematics describes how objects move. Dynamics goes further by examining why their motion changes. The central concept in dynamics is force, and the fundamental framework for ordinary mechanical motion is provided by Newton's laws of motion.
Dynamics is the branch of mechanics concerned with the relationship between the motion of bodies and the forces responsible for that motion.
Newton's laws provide a systematic way to analyse objects at rest, objects moving with constant velocity and objects undergoing acceleration.
4.2 Force and the Concept of Interaction
A force is an interaction that can change the state of motion of an object or deform it. Force is a vector quantity.
Examples include gravitational force, frictional force, normal reaction, tension, spring force and electric force.
The SI unit of force is the newton:
Forces may be broadly classified as contact forces and non-contact forces.
Contact Forces:
Contact forces arise from physical contact between bodies. Examples include friction, normal reaction and tension transmitted through a rope.
Non-Contact Forces:
Non-contact forces act without direct physical contact. Gravitational force is a major example and is sometimes described as an action-at-a-distance interaction in classical mechanics.
4.3 Newton's First Law of Motion
A body remains at rest or continues in uniform straight-line motion unless acted upon by a non-zero resultant external force.
The law identifies zero net force as the condition for constant velocity. Rest is simply the special case of constant velocity in which the velocity is zero.
If acceleration is zero, velocity remains constant.
A book resting on a table does not have zero forces acting on it. Its weight acts downward, while the table exerts an upward normal force of equal magnitude. The resultant force is zero, so the book remains at rest.
4.4 Inertia and Inertial Frames
Inertia is the tendency of an object to resist any change in its state of rest or uniform straight-line motion.
Mass is a measure of translational inertia. An object with greater mass requires a greater net force to produce the same acceleration.
An inertial frame is a reference frame in which Newton's first law is valid. Such a frame is either at rest or moves with constant velocity relative to another inertial frame.
An accelerating reference frame is generally non-inertial. In such a frame, additional apparent or fictitious forces may have to be introduced if Newton's laws are to be used in their familiar form.
4.5 Newton's Second Law of Motion
Newton's second law gives the quantitative relationship between force and acceleration.
The resultant external force on a body is equal to the time rate of change of its momentum.
For constant mass,
so
Therefore,
This equation means that acceleration has the direction of the resultant force.
Question: A net horizontal force of 24 N acts on a 6 kg object. Find its acceleration.
Given:
Required: Acceleration.
Formula:
Solution:
Answer: The acceleration is 4 m/s2 in the direction of the net force.
Question: Two horizontal forces of 50 N east and 20 N west act on a 10 kg block. Find the acceleration.
Solution:
Taking east as positive, the resultant force is
Therefore,
Answer: The block accelerates at 3 m/s2 east.
4.6 Mass, Weight and Gravitational Force
Mass and weight are related but physically distinct quantities.
Mass is a measure of the inertia of a body and the amount of matter it contains. In classical mechanics, it is treated as a scalar quantity and is measured in kilograms.
Weight is the gravitational force exerted on a body.
Near the Earth's surface, g≈9.8m/s2.
| Mass | Weight |
|---|---|
| Measure of inertia | Gravitational force |
| Scalar quantity | Vector quantity |
| Measured in kilograms | Measured in newtons |
| Approximately constant for a given body in classical mechanics | Depends on local gravitational field strength |
Question: Find the weight of a 70 kg person at a place where g=9.8 m/s2.
Formula:
Solution:
Answer: The person's weight is 686 N downward.
4.7 Newton's Third Law of Motion
When one body exerts a force on a second body, the second body simultaneously exerts an equal-magnitude force in the opposite direction on the first body.
If body A exerts a force on body B,
The two forces act on different bodies. This is why they do not cancel each other when analysing the motion of one body alone.
When a person pushes a wall, the person exerts a force on the wall and the wall exerts an equal and opposite force on the person. The pair constitutes a third-law interaction.
4.8 Free-Body Diagrams
A free-body diagram is a simplified representation of an isolated object showing all external forces acting on that object.
A reliable Newtonian analysis usually begins by isolating the object and identifying the forces acting on it. Typical forces include:
- weight mg acting vertically downward;
- normal reaction N perpendicular to a supporting surface;
- friction f along a surface;
- tension T along a string or rope;
- applied forces;
- spring forces where applicable.
Do not draw forces that the object exerts on other bodies. Draw only the forces acting on the object being analysed. Choose coordinate axes that make the equations as simple as possible.
4.9 Normal Reaction and Contact Forces
The normal reaction is the contact force exerted by a surface on an object, directed perpendicular to the surface.
For a body resting on a horizontal surface with no other vertical forces,
However, N is not always equal to mg. Other vertical forces or vertical acceleration can change its value.
Question: A 15 kg box rests on a horizontal floor. Find the normal reaction exerted by the floor. Take g=9.8m/s2.
Solution:
The box has no vertical acceleration, so
Answer: The normal reaction is 147 N upward.
4.10 Friction
Friction is a contact force that opposes relative motion or the tendency of relative motion between surfaces in contact.
Static Friction:
Static friction acts when there is no sliding between the surfaces. It adjusts in magnitude up to a limiting value:
The maximum static friction is
Kinetic Friction:
When surfaces slide relative to each other, the kinetic friction is commonly modelled as
Here μs and μk are coefficients of static and kinetic friction respectively.
Question: A 10 kg block slides on a horizontal surface with coefficient of kinetic friction 0.20. Find the frictional force. Take g=9.8m/s2.
Given:
Solution:
On a horizontal surface with no other vertical forces,
Then,
Answer: The kinetic frictional force has magnitude 19.6 N and acts opposite to the sliding motion.
4.11 Motion on Horizontal Surfaces
For a body moving along a horizontal surface, Newton's second law is applied separately in the horizontal and vertical directions.
Question: A 12 kg block is pulled horizontally by a force of 50 N across a rough surface. The coefficient of kinetic friction is 0.25. Find its acceleration. Take g=9.8m/s2.
Given:
Vertical Direction:
Friction:
Horizontal Resultant Force:
Acceleration:
Answer: The acceleration is approximately 1.72 m/s2.
Question: A 5 kg block on a smooth horizontal surface is acted on by a force of 40 N at 30° above the horizontal. Find its horizontal acceleration and the normal reaction. Take g=9.8m/s2.
Resolve the Applied Force:
Horizontal Motion:
Vertical Direction:
There is no vertical acceleration, so
Answer: Horizontal acceleration ≈ 6.93 m/s2; normal reaction = 29 N.
4.12 Motion on Inclined Planes
When a body is on an inclined plane, it is often convenient to choose one coordinate axis parallel to the plane and another perpendicular to it.
For a plane inclined at angle θ to the horizontal, the weight mg has components:
parallel to the plane, and
perpendicular to the plane.
If no other force has a perpendicular component,
Question: A 6 kg block slides down a smooth plane inclined at 30° to the horizontal. Find its acceleration. Take g=9.8m/s2.
Force Parallel to Plane:
Using F=ma,
Cancel m:
Answer: The block accelerates down the plane at 4.9 m/s2.
Question: A 10 kg block slides down a plane inclined at 25°. The coefficient of kinetic friction is 0.15. Find its acceleration. Take g=9.8m/s2.
Normal Reaction:
Friction:
Down-Slope Component of Weight:
Net Force Down the Plane:
Acceleration:
Answer: The block accelerates down the plane at approximately 2.81 m/s2.
4.13 Tension and Connected Particles
Tension is the pulling force transmitted through a stretched string, rope or cable. In idealized mechanics problems, a light inextensible string and a frictionless pulley are often assumed.
For a massless string passing over an ideal pulley, the tension is taken to have the same magnitude throughout the string.
Question: Two masses of 6 kg and 4 kg are connected by a light string passing over a frictionless pulley. Find the acceleration of the system and the tension in the string. Take g=9.8m/s2.
Given:
The 6 kg mass moves downward and the 4 kg mass moves upward.
For the 6 kg Mass:
For the 4 kg Mass:
Add the equations:
Now use
Answer: Acceleration = 1.96 m/s2; tension = 47.04 N.
Question: Two blocks of masses 3 kg and 5 kg are connected by a light horizontal string on a smooth surface. A horizontal force of 24 N pulls the 5 kg block. Find the acceleration and the tension in the string.
Whole System:
For the 3 kg Block:
The only horizontal force on it is the tension:
Answer: Acceleration = 3 m/s2; tension = 9 N.
4.14 Elevators and Apparent Weight
The reading of a weighing scale in an accelerating elevator is determined by the normal reaction rather than directly by the gravitational force. This normal reaction is often called the apparent weight.
Elevator Accelerating Upward:
Therefore,
Elevator Accelerating Downward:
Therefore,
Elevator Moving with Constant Velocity:
If acceleration is zero,
Free Fall:
If the elevator and person are both in free fall with acceleration g,
The person is then apparently weightless, although gravity is still acting.
Question: A 60 kg person stands on a scale in an elevator accelerating upward at 2 m/s2. Find the scale reading. Take g=9.8m/s2.
Formula:
Solution:
Answer: The scale reads 708 N.
Question: The same 60 kg person is in an elevator accelerating downward at 2 m/s2. Find the scale reading.
Formula:
Solution:
Answer: The scale reads 468 N.
4.15 Force as Action at a Distance
Some forces arise through direct contact, whereas others act between separated bodies. Gravity is the major example considered in mechanics.
In classical Newtonian mechanics, gravitational attraction is described as a force acting between masses even when they are not in physical contact. The quantitative law of universal gravitation will be developed later in this course.
The distinction between contact and non-contact interactions helps in constructing free-body diagrams. A body may experience several forces simultaneously, and the motion is determined by their vector sum.
4.16 Applications of Newtonian Mechanics
The general strategy for solving Newtonian mechanics problems is to translate a physical situation into a force model and then apply Newton's second law.
A practical sequence is:
- identify the object or system to be analysed;
- choose suitable coordinate directions;
- draw or mentally construct a free-body diagram;
- resolve forces into components if necessary;
- calculate the resultant force in each direction;
- apply ΣF=ma separately along the chosen axes;
- solve the resulting equations and interpret the signs physically.
Question: A 20 kg crate is pushed horizontally with a force of 100 N across a floor. A frictional force of 35 N opposes the motion. If the crate starts from rest, find its acceleration and speed after 4 s.
Resultant Force:
Acceleration:
Speed after 4 s:
Since the crate starts from rest, u=0.
Answer: Acceleration = 3.25 m/s2; speed after 4 s = 13 m/s.
Question: A 4 kg block rests on a horizontal surface. The coefficient of static friction is 0.40. What is the largest horizontal force that can be applied without causing the block to move? Take g=9.8m/s2.
Normal Reaction:
Maximum Static Friction:
Static friction can balance an applied force only up to this value.
Answer: The largest horizontal force that can be applied without causing motion is 15.68 N.
Question: A 5 kg block is pulled up a smooth plane inclined at 30° by a force of 40 N parallel to the plane. Find its acceleration. Take g=9.8m/s2.
Component of Weight Down the Plane:
Resultant Force Up the Plane:
Acceleration:
Answer: The block accelerates up the plane at 3.1 m/s2.
Question: A horizontal force causes a 2 kg object initially at rest to accelerate at 5 m/s2. Find the resultant force and the object's velocity after 6 s.
Resultant Force:
Velocity:
Answer: Resultant force = 10 N; velocity after 6 s = 30 m/s.
Newton's second law and the equations of kinematics are often used together. Newton's laws determine the acceleration from the forces, while the kinematic equations use that acceleration to determine velocity, displacement or time.
Chapter Summary
- Dynamics studies the relationship between forces and motion.
- A force is a vector interaction capable of changing motion or causing deformation.
- Newton's first law states that a body remains at rest or in uniform straight-line motion when the resultant external force is zero.
- Inertia is the tendency of a body to resist changes in its state of motion.
- An inertial frame is a reference frame in which Newton's first law holds.
- Newton's second law is fundamentally ΣF=dp/dt; for constant mass it becomes ΣF=ma.
- Mass measures inertia, while weight is the gravitational force W=mg.
- Newton's third law states that interaction forces occur in equal-magnitude, opposite-direction pairs acting on different bodies.
- Free-body diagrams identify all external forces acting on a selected body.
- The normal reaction acts perpendicular to a supporting surface.
- Static friction prevents sliding up to a limiting value, while kinetic friction acts during sliding.
- On an inclined plane, the components of weight are mg sinθ parallel to the plane and mg cosθ perpendicular to it.
- Tension transmits pulling forces through strings or ropes and can be analysed using Newton's laws.
- The normal reaction measured by a scale in an accelerating elevator represents apparent weight.
- Gravitational force is a non-contact interaction and is treated classically as an action-at-a-distance force.
- Newtonian mechanics problems are solved by identifying forces, resolving them into appropriate directions and applying ΣF=ma.
CHAPTER FIVE
Momentum, Impulse and Conservation of Linear Momentum
5.1 Introduction to Momentum
Newton's laws show that forces produce changes in motion. However, velocity alone does not completely describe how difficult it is to stop or redirect a moving object. A small object and a very massive object may have the same velocity, yet their responses during interactions can be very different. The quantity that combines mass and velocity is called linear momentum.
Momentum is especially useful when studying collisions, explosions, recoil and interactions that occur over short intervals of time. It also leads to one of the most important conservation principles in mechanics: the conservation of linear momentum.
5.2 Linear Momentum
The linear momentum of a particle is the product of its mass and velocity.
Momentum is a vector quantity because velocity is a vector. Its direction is therefore the same as the direction of the velocity.
The SI unit of momentum is
The dimensions of momentum are
Question: A car of mass 1200 kg moves east at 20 m/s. Determine its momentum.
Given:
Formula:
Solution:
Answer: The momentum is 2.4×104 kg m/s east.
Question: A 0.15 kg ball moves west at 30 m/s. Taking east as positive, find its momentum.
Solution:
Since west is negative,
Answer: The momentum is -4.5 kg m/s, or equivalently 4.5 kg m/s west.
5.3 Newton's Second Law in Momentum Form
The most general elementary form of Newton's second law expresses force as the rate of change of momentum:
For a body of constant mass,
Therefore,
Since dv/dt=a,
Thus, the familiar equation F=ma follows from the momentum formulation when mass is constant.
Question: The momentum of an object changes from 10 kg m/s east to 34 kg m/s east in 6 s. Find the average resultant force.
Formula:
Solution:
Answer: The average resultant force is 4 N east.
5.4 Impulse
Impulse is the product of a force and the time interval for which it acts when the force is constant.
The SI unit of impulse is newton-second, N s. Since
impulse has the same dimensions as momentum.
If force varies with time, impulse is more generally
Graphically, impulse is represented by the signed area under a force-time graph.
5.5 Impulse-Momentum Theorem
From Newton's second law,
For a constant force acting over a time interval Δt,
Hence,
The impulse of the resultant force acting on a body equals the change in the body's linear momentum.
Question: A constant force of 40 N acts on an object for 0.25 s. Calculate the impulse.
Formula:
Solution:
Answer: The impulse is 10 N s.
Question: A 0.20 kg ball moving east at 15 m/s is struck and leaves westward at 25 m/s. Find the impulse on the ball.
Given: Take east as positive.
Formula:
Solution:
Answer: The impulse is 8 N s west.
Question: A 0.5 kg ball initially at rest receives an impulse of 6 N s. Find its final speed.
Formula:
Solution: Since u=0,
Answer: The final speed is 12 m/s.
For a given change in momentum, increasing the time over which the change occurs reduces the average force. This principle explains the protective function of airbags, seat belts, crash cushions, helmets and padded landing surfaces.
5.6 Conservation of Linear Momentum
Consider a system of interacting particles. Internal forces occur in Newton's third-law pairs. If the net external force on the system is zero, the total momentum of the system remains constant.
If the resultant external force on a system is zero, the total linear momentum of the system remains constant.
For two bodies moving along one straight line,
Question: A 4 kg trolley moving at 6 m/s collides with a stationary 2 kg trolley. They stick together. Find their common velocity after collision.
Given:
Formula:
Solution:
Answer: Their common velocity is 4 m/s in the original direction of the 4 kg trolley.
5.7 Systems of Particles
Many physical objects and mechanical systems consist of several particles. Instead of treating each particle independently in every situation, it is often useful to consider the system as a whole.
For a system containing particles with momenta p1, p2, ..., the total momentum is the vector sum
Internal forces may change the momenta of individual particles, but they do not change the total momentum of an isolated system.
5.8 Centre of Mass
The centre of mass of a system is the mass-weighted average position of all the particles making up the system.
For particles arranged along the x-axis,
More compactly,
In three dimensions, the centre-of-mass position vector is
where M=Σmi is the total mass.
Question: A 2 kg particle is at x=1 m and a 6 kg particle is at x=5 m. Find the centre of mass.
Formula:
Solution:
Answer: The centre of mass is at x=4 m.
5.9 Motion of the Centre of Mass
The total momentum of a system can be expressed in terms of the velocity of its centre of mass:
The resultant external force determines the acceleration of the centre of mass:
Consequently, if the resultant external force is zero,
and the centre of mass remains at rest or moves with constant velocity.
Question: A system has total mass 20 kg and total momentum 100 kg m/s east. Find the velocity of its centre of mass.
Formula:
Solution:
Answer: The centre of mass moves at 5 m/s east.
5.10 Collisions
A collision is an interaction in which two or more bodies exert relatively large forces on one another over a relatively short time interval. During the collision, the bodies may change their velocities, directions or shapes.
If external impulse during the collision is negligible, total momentum is conserved:
Momentum conservation does not require kinetic energy to remain constant. The behaviour of kinetic energy distinguishes important types of collision.
5.11 Elastic and Inelastic Collisions
Elastic Collision:
An elastic collision is a collision in which both total linear momentum and total kinetic energy are conserved.
Inelastic Collision:
An inelastic collision is one in which total momentum is conserved for an isolated system but kinetic energy is not conserved.
In a perfectly inelastic collision, the colliding bodies stick together and move with a common final velocity.
Question: A 3 kg body moving at 8 m/s collides with a stationary 5 kg body. They stick together. Find their final velocity and determine the kinetic energy lost.
Momentum Conservation:
Initial Kinetic Energy:
Final Kinetic Energy:
Kinetic Energy Lost:
Answer: Final velocity = 3 m/s; kinetic energy lost = 60 J.
Question: A 2 kg object moving at 6 m/s collides head-on elastically with an identical stationary object. The first object stops after the collision. Find the velocity of the second object.
Momentum Conservation:
Answer: The second object moves at 6 m/s in the original direction of the first object.
5.12 Explosions and Recoil
Momentum conservation also applies when a system initially together separates into parts. Such processes include explosions and recoil.
If an isolated system is initially at rest, its total momentum is zero. Therefore,
Question: A stationary object of mass 10 kg explodes into two fragments of masses 4 kg and 6 kg. The 4 kg fragment moves east at 9 m/s. Find the velocity of the 6 kg fragment.
Initial Momentum:
Take east as positive:
Answer: The 6 kg fragment moves at 6 m/s west.
Question: A rifle of mass 5 kg fires a bullet of mass 0.02 kg at 400 m/s. If the rifle and bullet were initially at rest, find the recoil velocity of the rifle.
Solution:
Take the bullet's direction as positive:
Answer: The rifle recoils at 1.6 m/s opposite to the bullet's motion.
5.13 Momentum in Two Dimensions
Because momentum is a vector, conservation of momentum applies independently to perpendicular components.
This principle is useful for oblique collisions, explosions and situations in which objects move in different directions after interaction.
Question: A stationary object explodes into two fragments. One fragment has momentum 12 kg m/s east and the other has momentum 5 kg m/s north. What momentum must the remaining fragment have if the original total momentum was zero?
Solution:
The first two fragments have resultant momentum
To make total momentum zero, the remaining fragment must have the opposite momentum:
Its magnitude is
Answer: The required momentum has magnitude 13 kg m/s and is directed opposite to the resultant of the other two momenta.
5.14 Applications of Momentum and Impulse
Momentum and impulse provide powerful methods for analysing interactions in which forces may be large but act for short periods. Important applications include vehicle collisions, sports, rocket propulsion, recoil and impact protection.
Question: A 1000 kg car moving at 20 m/s is brought to rest. Compare the average stopping force when it stops in 0.10 s and when it stops in 0.50 s.
Change in Momentum:
First Stopping Time:
Second Stopping Time:
Answer: The average force magnitudes are 200,000 N and 40,000 N. Increasing the stopping time from 0.10 s to 0.50 s reduces the average force by a factor of five.
Chapter Summary
- Linear momentum is defined by p=mv and is a vector quantity.
- Newton's second law may be written as ΣF=dp/dt.
- Impulse is the effect of force acting over a time interval and is equal to the change in momentum.
- For constant force, J=FΔt=Δp.
- The area under a force-time graph represents impulse.
- Total linear momentum remains constant when the resultant external force or external impulse on a system is zero.
- The total momentum of a system is the vector sum of the momenta of its particles.
- The centre of mass is the mass-weighted average position of a system.
- The total momentum of a system can be expressed as P=Mvcm.
- Momentum is conserved in isolated elastic and inelastic collisions.
- Kinetic energy is conserved in elastic collisions but not generally in inelastic collisions.
- In a perfectly inelastic collision, the colliding bodies move together after impact.
- Recoil and explosions are explained using conservation of momentum.
- In two dimensions, momentum conservation must be applied separately to each component.
CHAPTER SIX
Work, Energy and Conservation of Energy
6.1 Introduction to Work and Energy
Newton's laws provide a direct method for analysing motion through forces and acceleration. Many mechanical problems, however, can be solved more efficiently by considering work and energy. Energy methods are particularly useful when the details of acceleration at every instant are not required.
Energy is a scalar quantity. This makes energy calculations different from force and momentum calculations, where direction must be handled explicitly as part of a vector.
Energy is the capacity of a physical system to produce change or perform work. In mechanics, important forms include kinetic energy and potential energy.
The SI unit of both work and energy is the joule:
6.2 Work Done by a Constant Force
When a constant force causes an object to undergo displacement, the work done depends on the component of the force in the direction of displacement.
The work done by a constant force is the scalar product of the force and displacement.
Using the definition of the scalar product,
where θ is the angle between the force and displacement.
Question: A horizontal force of 50 N moves a box through a horizontal distance of 8 m. Find the work done by the force.
Given:
Formula:
Solution:
Answer: The work done is 400 J.
Question: A force of 100 N acts at 60° to the horizontal while an object moves horizontally through 5 m. Calculate the work done by the force.
Formula:
Solution:
Answer: The work done is 250 J.
6.3 Positive, Negative and Zero Work
The sign of work depends on the angle between force and displacement.
| Angle | Nature of Work | Physical Interpretation |
|---|---|---|
| 0°≤θ<90° | Positive | Force has a component in the direction of displacement. |
| θ=90° | Zero | Force is perpendicular to displacement. |
| 90°<θ≤180° | Negative | Force has a component opposite to displacement. |
Friction commonly does negative work on a sliding body because the frictional force acts opposite to the displacement.
Question: A frictional force of 20 N acts opposite to the motion of a block that moves 10 m. Find the work done by friction.
Given:
Solution:
Answer: The work done by friction is -200 J.
When an object moves horizontally at constant height, its weight acts vertically downward. Since weight is perpendicular to the horizontal displacement, gravity does zero work during that horizontal displacement.
6.4 Work Done by a Variable Force
If force varies with position, the simple expression W=Fs cosθ cannot generally be applied using a single constant value of force. In one-dimensional motion, the work done from position x1 to x2 is
The work is therefore represented by the signed area under the force-position graph.
Question: A force varies with position according to F(x)=4x newtons. Find the work done as the object moves from x=0 to x=3 m.
Formula:
Solution:
Answer: The work done is 18 J.
6.5 Kinetic Energy
Kinetic energy is the energy possessed by a body because of its motion.
Kinetic energy is a scalar and is never negative in classical mechanics because it depends on the square of speed.
Question: Calculate the kinetic energy of a 1500 kg car moving at 20 m/s.
Formula:
Solution:
Answer: The kinetic energy is 3.0×105 J.
Kinetic energy is proportional to the square of speed. If the speed of an object doubles while its mass remains constant, its kinetic energy becomes four times as large.
6.6 The Work-Energy Theorem
The net work done on a particle equals the change in its kinetic energy.
Therefore,
This theorem establishes a direct connection between force, displacement and change in speed.
Question: A 4 kg object initially moving at 3 m/s has 50 J of net work done on it. Find its final speed.
Initial Kinetic Energy:
Work-Energy Theorem:
Now,
Answer: The final speed is approximately 5.83 m/s.
Question: A 1000 kg car moving at 15 m/s is brought to rest by braking forces. Determine the net work done on the car.
Formula:
Solution:
Answer: The net work done is -1.125×105 J.
6.7 Potential Energy
Potential energy is energy associated with the position or configuration of a system when conservative forces are involved.
For a conservative force, the change in potential energy is defined by
Thus, when a conservative force does positive work, the associated potential energy decreases; when it does negative work, potential energy increases.
6.8 Gravitational Potential Energy Near the Earth's Surface
Near the Earth's surface, where gravitational acceleration can be treated as approximately constant, the change in gravitational potential energy is
If the zero level of potential energy is chosen at h=0, then
Only differences in potential energy have direct physical significance; the zero level may be chosen conveniently.
Question: A 5 kg object is raised vertically through 8 m. Find the increase in gravitational potential energy. Take g=9.8m/s2.
Formula:
Solution:
Answer: The gravitational potential energy increases by 392 J.
6.9 Elastic Potential Energy
An ideal spring obeys Hooke's law within its elastic limit:
where k is the spring constant and x is the displacement from equilibrium. The negative sign indicates that the spring force acts opposite to the displacement.
The elastic potential energy stored in an ideal spring is
Question: A spring of force constant 200 N/m is compressed by 0.10 m. Find the elastic potential energy stored.
Given:
Formula:
Solution:
Answer: The spring stores 1 J of elastic potential energy.
6.10 Conservative and Non-Conservative Forces
A force is conservative if the work it does between two points is independent of the path followed and depends only on the initial and final positions.
For a conservative force, the work done around any closed path is zero:
Examples include gravitational force and the force of an ideal spring.
A non-conservative force is one for which the work done generally depends on the path followed.
Kinetic friction is an important example. Mechanical energy converted by friction may appear as thermal energy and other internal forms.
| Conservative Forces | Non-Conservative Forces |
|---|---|
| Work is path independent. | Work generally depends on the path. |
| Potential energy can be associated with the force. | A single-valued potential-energy function generally cannot be assigned in the same way. |
| Work around a closed path is zero. | Work around a closed path need not be zero. |
| Examples: gravity, ideal spring force. | Example: kinetic friction. |
6.11 Conservation of Mechanical Energy
Mechanical energy is the sum of kinetic and potential energies:
When only conservative forces do work,
When only conservative forces perform work on a system, the total mechanical energy of the system remains constant.
Question: A stone is released from rest at a height of 20 m above the ground. Neglect air resistance. Find its speed just before reaching the ground. Take g=9.8m/s2.
Initial Energy:
Final Energy:
By conservation of mechanical energy,
Cancel m:
Answer: The speed just before reaching the ground is approximately 19.8 m/s.
Question: A ball is projected vertically upward at 14 m/s. Neglect air resistance. Use conservation of energy to determine its maximum height above the point of projection. Take g=9.8m/s2.
Initial Energy:
At maximum height the instantaneous speed is zero, so the gain in gravitational potential energy equals the initial kinetic energy:
Cancel m:
Answer: The maximum height is 10 m.
Question: A 2 kg block is released from rest and slides down a smooth track through a vertical height of 5 m. Find its speed at the bottom. Take g=9.8m/s2.
Solution:
Answer: The speed at the bottom is approximately 9.90 m/s.
6.12 Energy in the Presence of Non-Conservative Forces
Mechanical energy is not generally conserved when non-conservative forces such as friction perform work. The change in mechanical energy is related to the work done by non-conservative forces:
This does not violate the broader conservation of energy. Energy may be transformed from mechanical energy into thermal energy, sound, deformation or other forms.
Question: A 5 kg block initially moving at 10 m/s slides along a horizontal rough surface and stops after 8 m. Determine the average frictional force.
Initial Kinetic Energy:
Final Kinetic Energy:
Therefore,
Since friction acts opposite to displacement,
Answer: The average frictional force has magnitude 31.25 N.
6.13 Power
Power is the rate at which work is done or energy is transferred.
Average power is
Instantaneous power is
Since dW=F·dr,
For a force parallel to velocity,
The SI unit of power is the watt:
Question: A machine performs 24,000 J of work in 30 s. Find its average power.
Formula:
Solution:
Answer: The average power is 800 W.
Question: A car experiences a driving force of 2500 N while moving at a constant speed of 20 m/s. Determine the power delivered by the driving force.
Formula:
Solution:
Answer: The power delivered is 50 kW.
Question: A motor lifts a 200 kg load vertically through 15 m in 10 s at constant speed. Find the useful power output. Take g=9.8m/s2.
Work Done:
Power:
Answer: The useful power output is 2940 W or 2.94 kW.
6.14 Efficiency
Real machines do not normally convert all supplied energy into useful output. Some energy is transferred into unwanted forms such as thermal energy and sound.
Efficiency is the ratio of useful energy output to total energy input, or equivalently useful power output to total power input.
Alternatively,
Question: A machine receives 5000 J of energy and delivers 3750 J as useful work. Determine its efficiency.
Formula:
Solution:
Answer: The machine is 75% efficient.
6.15 Applications of Work and Energy Principles
The work-energy method can often replace a lengthy force-and-acceleration analysis. Instead of calculating acceleration and then applying the equations of motion, the initial and final energy states can sometimes be related directly.
Question: A 2 kg block starts from rest and is pushed by a constant horizontal force of 10 N through 5 m on a smooth horizontal surface. Find its final speed using the work-energy theorem.
Work Done:
Work-Energy Theorem:
Since the block starts from rest, Ki=0.
Answer: The final speed is approximately 7.07 m/s.
Question: A 3 kg object starts from rest at the top of a smooth slope 12 m above its lowest point. Find its speed at the bottom. Take g=9.8m/s2.
Principle: Since the slope is smooth, mechanical energy is conserved.
Mass cancels:
Answer: The speed at the bottom is approximately 15.34 m/s.
Question: A 1000 kg car climbs a hill of vertical height 50 m at constant speed. Determine the increase in gravitational potential energy. If this is accomplished in 25 s, determine the minimum average power required to increase the car's gravitational potential energy. Take g=9.8m/s2.
Potential Energy Increase:
Average Power:
Answer: The increase in gravitational potential energy is 4.90×105 J, and the corresponding minimum average power is 19.6 kW.
Newton's laws are especially useful when forces and accelerations are required. Energy methods are often more efficient when a problem asks for speed, height, displacement or energy changes between two states. Both approaches describe the same mechanics and should give consistent results when applied correctly.
Chapter Summary
- Work is the scalar product of force and displacement: W=Fs cosθ.
- Work is positive when a force assists displacement, negative when it opposes displacement and zero when force is perpendicular to displacement.
- For a variable one-dimensional force, work is W=∫F(x)dx.
- Kinetic energy is the energy associated with motion and is given by K=(1/2)mv2.
- The work-energy theorem states that net work equals the change in kinetic energy.
- Potential energy is associated with position or configuration when conservative forces are involved.
- Near the Earth's surface, the change in gravitational potential energy is ΔU=m g Δh.
- An ideal spring stores elastic potential energy U=(1/2)kx2.
- Conservative forces do path-independent work and can be associated with potential-energy functions.
- When only conservative forces do work, total mechanical energy K+U remains constant.
- Non-conservative forces can change the mechanical energy of a system while total energy remains conserved when all forms of energy are considered.
- Power is the rate of doing work or transferring energy and is measured in watts.
- Instantaneous mechanical power can be expressed as P=F·v.
- Efficiency compares useful output with total input and is commonly expressed as a percentage.
- Work-energy and conservation-of-energy methods provide efficient alternatives to direct force-and-acceleration calculations in many mechanics problems.
CHAPTER NINE
Circular Motion and Moment of Inertia
9.1 Introduction to Circular Motion
Circular motion occurs whenever an object moves along a circular path. Examples include a stone tied to a string and whirled in a circle, a vehicle travelling around a curved road, a rotating wheel, the blades of a fan and, approximately, a satellite moving in a circular orbit.
Circular motion is important because the direction of the velocity changes continuously even when the speed remains constant. Since acceleration is the rate of change of velocity, an object moving at constant speed in a circle is still accelerating.
Circular motion is the motion of a body or particle along a path whose distance from a fixed centre remains constant.
The fixed distance between the moving particle and the centre of the circle is the radius r.
9.2 Angular and Linear Description of Circular Motion
A particle moving along a circle can be described by either its angular displacement θ or the arc length s travelled along the circumference.
When θ is measured in radians,
Differentiating with respect to time gives
where v is the tangential speed and ω is the angular speed.
Question: A wheel of radius 0.50 m rotates through an angle of 8 rad. Find the distance travelled by a point on its rim.
Given:
Required: Arc length s.
Formula:
Solution:
Answer: The point travels a distance of 4 m.
9.3 Period and Frequency
The period T is the time required for one complete revolution or cycle.
The frequency f is the number of complete revolutions or cycles made per unit time.
The SI unit of frequency is the hertz, Hz, equivalent to s-1.
Period and frequency are reciprocals:
and
Since one complete revolution corresponds to 2π radians,
Consequently,
Question: A rotating wheel completes 120 revolutions in one minute. Determine its frequency, period and angular speed.
Solution:
Convert the number of revolutions per minute to revolutions per second:
The period is
The angular speed is
Answer: Frequency = 2 Hz; period = 0.50 s; angular speed = 4π rad/s ≈ 12.57 rad/s.
9.4 Uniform Circular Motion
Uniform circular motion is motion along a circular path at constant speed.
The word uniform refers to the magnitude of the velocity, not to the velocity vector itself. Velocity has both magnitude and direction. Although the speed remains constant, the direction of the velocity changes continuously.
At every point on a circular path, the instantaneous velocity is tangent to the circle. The acceleration responsible for changing the direction of the velocity points toward the centre.
Constant speed does not necessarily mean zero acceleration. In uniform circular motion, speed is constant but velocity changes because its direction changes. The particle therefore possesses acceleration.
9.5 Centripetal Acceleration
Centripetal acceleration is the inward acceleration of an object moving along a circular path. It is always directed toward the centre of the circle.
Its magnitude is
Using v=rω,
Using ω=2π/T,
In terms of frequency,
Question: A particle moves in a circle of radius 2 m at a constant speed of 6 m/s. Find its centripetal acceleration.
Given:
Formula:
Solution:
Answer: The centripetal acceleration is 18 m/s2, directed toward the centre.
Question: A point on a rotating disc is 0.40 m from the axis and rotates at 10 rad/s. Determine its centripetal acceleration.
Formula:
Solution:
Answer: The centripetal acceleration is 40 m/s2.
9.6 Centripetal Force
According to Newton's second law, an acceleration requires a resultant force. Therefore, the inward centripetal acceleration in circular motion requires a resultant inward force.
Centripetal force is the name given to the resultant force directed toward the centre of a circular path that produces centripetal acceleration.
From Newton's second law,
Therefore,
or
Centripetal force is not an additional fundamental force. Depending on the physical situation, the inward force may be supplied by tension, friction, gravity, a normal reaction, or a combination of forces.
Question: A 0.50 kg stone moves in a horizontal circle of radius 1.5 m at 6 m/s. Determine the required centripetal force.
Formula:
Solution:
Answer: The required inward force is 12 N.
9.7 Applications of Circular Motion
Circular motion appears in many physical situations. The essential method of analysis is to identify the force or combination of forces whose inward component provides the required centripetal force.
Vehicle Moving on a Level Circular Road:
For a vehicle turning on a level road, static friction between the tyres and road can provide the horizontal centripetal force.
If the maximum static friction is fmax=μsN and N=mg, then
Hence the maximum speed before slipping is
Question: A car moves around a level circular bend of radius 50 m. If the coefficient of static friction between the tyres and road is 0.40, estimate the maximum speed without skidding. Take g=9.8 m/s2.
Formula:
Solution:
Answer: The maximum speed is approximately 14 m/s.
Conical Pendulum:
In a conical pendulum, a mass attached to a string moves in a horizontal circle while the string makes a constant angle θ with the vertical.
The vertical component of tension balances the weight:
The horizontal component supplies the centripetal force:
Dividing the equations gives
9.8 Banking of Roads
A road is banked when its outer edge is raised above its inner edge. Banking allows part of the normal reaction from the road to contribute toward the centripetal force required for turning.
For an ideal banked road in which friction is not required, let θ be the banking angle. Resolving the normal force,
and
Dividing,
Therefore,
Question: A frictionless road of radius 80 m is banked at 15°. Find the speed for which no sideways friction is required. Take g=9.8 m/s2.
Formula:
Solution:
Answer: The design speed is approximately 14.5 m/s.
9.9 Vertical Circular Motion
When an object moves in a vertical circle, gravity contributes differently to the radial force at different positions. Consequently, the speed generally changes unless an external mechanism maintains it.
Consider a mass attached to a light string moving in a vertical circle of radius r.
At the Bottom of the Circle:
The inward direction is upward, so
Therefore,
At the Top of the Circle:
Both tension and weight may act toward the centre:
For a string to remain just taut at the top, the limiting condition is T=0. Therefore,
and
Question: A 0.20 kg mass moves at 5 m/s at the bottom of a vertical circle of radius 1 m. Find the tension in the string at that instant. Take g=9.8 m/s2.
Formula:
Solution:
Answer: The tension is 6.96 N.
9.10 Introduction to Moment of Inertia
In translational motion, mass measures a body's resistance to linear acceleration. In rotational motion, the corresponding quantity is moment of inertia.
The moment of inertia of a body about a specified axis is a measure of its resistance to angular acceleration about that axis.
Moment of inertia depends not only on the total mass but also on how that mass is distributed relative to the axis of rotation. Mass located farther from the axis contributes more strongly.
The SI unit of moment of inertia is
9.11 Moment of Inertia of a System of Particles
For a system consisting of discrete particles,
where ri is the perpendicular distance of the ith particle from the axis.
Question: Two particles of masses 2 kg and 3 kg are located 0.50 m and 0.80 m respectively from a fixed axis. Find the moment of inertia of the system.
Formula:
Solution:
Answer: The moment of inertia is 2.42 kg m2.
9.12 Moment of Inertia of Continuous Bodies
For a continuous body, the body may be imagined as being divided into very small mass elements dm. The moment of inertia is then
The exact result depends on the geometry of the body, its density distribution and the chosen axis.
Question: Derive the moment of inertia of a uniform thin rod of mass M and length L about an axis through its centre and perpendicular to the rod.
Given: The linear mass density is
A small element of length dx has mass
Formula:
Solution:
Answer: The moment of inertia is I=ML2/12.
9.13 Standard Moments of Inertia
The following expressions are useful for common uniform bodies. The axis must always be identified because moment of inertia depends on the axis of rotation.
| Body | Axis | Moment of Inertia |
|---|---|---|
| Thin ring or hoop, radius R | Through centre, perpendicular to plane | I=MR2 |
| Solid disc, radius R | Through centre, perpendicular to plane | I=(1/2)MR2 |
| Solid cylinder, radius R | Along symmetry axis | I=(1/2)MR2 |
| Thin rod, length L | Through centre, perpendicular to rod | I=(1/12)ML2 |
| Thin rod, length L | Through one end, perpendicular to rod | I=(1/3)ML2 |
| Solid sphere, radius R | Through centre | I=(2/5)MR2 |
| Thin spherical shell, radius R | Through centre | I=(2/3)MR2 |
Question: Find the moment of inertia of a uniform solid disc of mass 6 kg and radius 0.40 m about its central axis.
Formula:
Solution:
Answer: The moment of inertia is 0.48 kg m2.
9.14 Radius of Gyration
The radius of gyration of a body about an axis is the distance from the axis at which the entire mass of the body could be imagined to be concentrated without changing its moment of inertia.
If k is the radius of gyration,
Therefore,
Question: A body of mass 8 kg has moment of inertia 2 kg m2 about a certain axis. Find its radius of gyration.
Formula:
Solution:
Answer: The radius of gyration is 0.50 m.
9.15 Parallel-Axis Theorem
The parallel-axis theorem allows the moment of inertia about one axis to be obtained from the moment of inertia about a parallel axis through the centre of mass.
If Icm is the moment of inertia about an axis through the centre of mass, then the moment of inertia about a parallel axis a perpendicular distance d away is
Question: Use the parallel-axis theorem to obtain the moment of inertia of a uniform rod of length L about an axis through one end and perpendicular to the rod.
Given:
The distance from the centre to the end is
Solution:
Answer: The moment of inertia about the end is I=(1/3)ML2.
9.16 Perpendicular-Axis Theorem
For a thin planar lamina lying in the xy-plane, the perpendicular-axis theorem relates moments of inertia about three mutually perpendicular axes through the same point.
The theorem applies to planar bodies. The z-axis is perpendicular to the plane, while the x- and y-axes lie in the plane.
Question: A uniform circular disc has moment of inertia (1/2)MR2 about the axis through its centre perpendicular to its plane. Find its moment of inertia about a diameter.
Solution:
By symmetry,
Using the perpendicular-axis theorem,
Therefore,
Answer: The moment of inertia about a diameter is (1/4)MR2.
9.17 Rotational Dynamics and Moment of Inertia
Moment of inertia becomes dynamically important through Newton's second law for rotation:
For the same applied torque, a body with a larger moment of inertia develops a smaller angular acceleration. This is why both the quantity of mass and its distribution relative to the axis matter in rotational dynamics.
Question: A solid disc of mass 10 kg and radius 0.50 m is acted upon by a constant torque of 5 N m about its central axis. Determine its angular acceleration.
Moment of Inertia:
Rotational Dynamics:
Answer: The angular acceleration is 4 rad/s2.
Question: A uniform solid cylinder of mass 4 kg and radius 0.30 m rotates at 20 rad/s about its symmetry axis. Find its rotational kinetic energy.
Moment of Inertia:
Rotational Kinetic Energy:
Answer: The rotational kinetic energy is 36 J.
Chapter Summary
- Circular motion occurs when an object moves along a path of constant radius about a fixed centre.
- Arc length and angular displacement are related by s=rθ.
- Linear and angular speed are related by v=rω.
- Period and frequency satisfy T=1/f, while ω=2πf=2π/T.
- Uniform circular motion has constant speed but continuously changing velocity.
- Centripetal acceleration is directed toward the centre and has magnitude v2/r=ω2r.
- The required centripetal force is the resultant inward force, Fc=mv2/r.
- Friction, tension, gravity or normal reaction may supply the required centripetal force depending on the situation.
- Banking allows a component of the normal force to contribute to the centripetal force.
- Moment of inertia measures resistance to angular acceleration and depends on both mass and its distribution about the axis.
- For discrete particles, I=Σmr2; for continuous bodies, I=∫r2dm.
- Radius of gyration is defined through I=Mk2.
- The parallel-axis theorem is I=Icm+Md2.
- For a planar body, the perpendicular-axis theorem is Iz=Ix+Iy.
- Rotational dynamics is governed by Στ=Iα.
CHAPTER TEN
Gyroscopes, Precession and Advanced Rotational Dynamics
10.1 Introduction to Gyroscopic Motion
A rapidly spinning body can behave in ways that may at first appear surprising. A spinning wheel supported at one end of its axle may resist falling and instead rotate slowly about a vertical direction. A spinning top can remain upright for a considerable time, while a non-spinning top quickly falls.
These behaviours arise from angular momentum and the way an external torque changes the direction of the angular-momentum vector. The study of gyroscopes therefore provides an important application of rotational dynamics.
Gyroscopic motion is the characteristic rotational behaviour of a spinning body whose angular momentum responds to an applied torque, often by changing direction rather than simply falling in the direction of the torque.
10.2 Review of Angular Momentum
For a particle,
For a rigid body rotating about a fixed principal axis,
The magnitude is therefore
The direction of angular momentum is determined by the right-hand rule. Curl the fingers of the right hand in the direction of rotation; the extended thumb indicates the direction of the angular velocity and, for rotation about a principal axis, the angular momentum.
Question: A flywheel has moment of inertia 5 kg m2 and rotates at 30 rad/s. Determine its angular momentum.
Formula:
Solution:
Answer: The angular momentum has magnitude 150 kg m2/s.
10.3 Torque and Change of Angular Momentum
The fundamental connection between torque and angular momentum is
This equation shows that an external torque changes angular momentum. Because angular momentum is a vector, torque may change its magnitude, its direction, or both.
If the torque acts parallel to the angular momentum, it primarily changes the magnitude of L. If it acts perpendicular to L, it can primarily change the direction of the angular-momentum vector.
Question: A constant torque of 12 N m acts in the direction of the angular momentum of a rotating body for 5 s. Find the magnitude of the change in angular momentum.
Formula:
Solution:
Answer: The angular momentum changes in magnitude by 60 kg m2/s.
10.4 The Gyroscope
A gyroscope is a rapidly rotating body, commonly a wheel or disc, mounted so that its axis of rotation is able to change direction.
A basic gyroscope may consist of a wheel rotating about an axle. When the wheel spins rapidly, it possesses substantial angular momentum. The direction of the axle corresponds approximately to the direction of its angular momentum vector.
If no external torque acts, the angular momentum remains constant in both magnitude and direction. Consequently, the spin axis tends to maintain its orientation in inertial space.
When an external torque acts perpendicular to the angular momentum, the axis changes direction. This directional change produces precession.
10.5 Stability of a Spinning Body
The apparent stability of a rapidly spinning body is a consequence of its angular momentum. A large angular momentum requires a correspondingly significant torque acting over time to produce a large change in orientation.
Since
a body may possess large angular momentum because it has a large moment of inertia, a large angular speed, or both.
A stationary bicycle wheel is relatively easy to reorient. When the same wheel spins rapidly, changing the direction of its axle becomes more difficult because the wheel possesses substantial angular momentum.
This does not mean that a spinning body cannot change its orientation. It means that its response to an applied torque must be understood through the vector equation τ=dL/dt.
10.6 Precession
Precession is the relatively slow rotation of the spin axis of a rotating body about another direction as a result of an external torque.
Consider a rapidly spinning wheel supported at one end of its axle. Gravity acts downward at the centre of mass, producing a torque about the support point. Rather than simply causing the wheel to fall, this torque continuously changes the direction of the angular-momentum vector. The axle consequently sweeps around the vertical axis.
The angular velocity associated with this motion of the axis is called the precessional angular velocity and is commonly represented by Ω.
10.7 Precession of a Gyroscope Under Gravity
Suppose a gyroscope of mass M is supported at one end of its axle. Let the centre of mass be a distance l from the pivot. If the axle is horizontal, the magnitude of the gravitational torque is
For steady precession of a rapidly spinning gyroscope, the change in angular momentum is mainly a change in direction. If the angular momentum vector precesses at angular speed Ω, then for the horizontal-axis case,
Since
we obtain
Therefore,
For a given gyroscope and geometry, increasing the spin angular speed ω decreases the precession rate Ω. A rapidly spinning gyroscope therefore precesses more slowly than the same gyroscope spinning at a lower rate, under the assumptions of steady precession.
10.8 Gyroscopic Precession Rate
Question: A gyroscope has mass 2 kg, moment of inertia 0.10 kg m2, spin angular speed 100 rad/s, and its centre of mass is 0.20 m from the pivot. Find its steady precession angular speed when the axle is horizontal. Take g=9.8 m/s2.
Given:
Formula:
Solution:
Answer: The precession angular speed is approximately 0.392 rad/s.
Question: For the gyroscope in Worked Example 3, determine the period of precession.
Formula:
Solution:
Answer: The precession period is approximately 16.0 s.
Question: A gyroscope has angular momentum 40 kg m2/s. A perpendicular torque of magnitude 8 N m produces steady precession. Determine the precession rate for the geometry in which τ=ΩL.
Formula:
Solution:
Answer: The precession angular speed is 0.20 rad/s.
10.9 Nutation
Nutation is an oscillatory or nodding motion of the rotational axis that may accompany precession.
A gyroscope released under conditions that do not correspond exactly to steady precession may exhibit both precession and a periodic variation in the inclination of its axis. This additional oscillatory motion is nutation.
Thus, three rotational motions may occur simultaneously:
- Spin: rapid rotation of the body about its own symmetry axis.
- Precession: slower rotation of the spin axis about another direction.
- Nutation: oscillation of the inclination of the spin axis.
10.10 Conservation of Angular Momentum in Rotating Systems
When the resultant external torque on a system is zero,
so that
For a body rotating about a fixed axis, this often becomes
If the moment of inertia decreases while external torque remains negligible, the angular speed increases.
Question: A student on a rotating stool has a total moment of inertia of 6 kg m2 and rotates at 2 rad/s. After drawing the arms inward, the moment of inertia becomes 3 kg m2. Find the new angular speed.
Formula:
Solution:
Answer: The new angular speed is 4 rad/s.
Angular Momentum in Collisions:
Angular momentum conservation can also be applied when rotating objects interact over a short time and external torque about the chosen axis is negligible.
Question: A disc with moment of inertia 2 kg m2 rotates at 10 rad/s. A second non-rotating disc with moment of inertia 3 kg m2 is gently dropped onto it. The discs eventually rotate together. Find their common angular speed, assuming negligible external torque.
Initial Angular Momentum:
Final Angular Momentum:
By conservation of angular momentum,
Answer: The discs rotate together at 4 rad/s.
Angular momentum can be conserved even when rotational kinetic energy is not conserved. In the two-disc example, friction between the discs converts some mechanical energy into internal energy while the total angular momentum remains constant because the external torque is negligible.
10.11 Rolling Motion
A rolling object combines translation of its centre of mass with rotation about an axis through its centre of mass. A rolling wheel therefore has both linear velocity and angular velocity.
Rolling motion is the combined translational and rotational motion of a body as it moves over a surface.
A wheel rolling along a road illustrates this combination clearly. Its centre moves forward while the wheel simultaneously rotates.
10.12 Rolling Without Slipping
For pure rolling without slipping, the distance travelled by the centre of mass is equal to the arc length rolled along the circumference:
Differentiating with respect to time gives
Differentiating again gives, for the corresponding tangential acceleration relation,
For rolling without slipping, the translational speed of the centre of mass and the angular speed satisfy vcm=Rω.
Question: A wheel of radius 0.40 m rolls without slipping at a centre-of-mass speed of 8 m/s. Find its angular speed.
Formula:
Solution:
Answer: The angular speed is 20 rad/s.
Velocity of Points on a Rolling Wheel:
For a wheel rolling without slipping on a stationary horizontal surface, the instantaneous velocity of a point on the wheel is obtained by combining the translational velocity of the centre with the velocity of that point relative to the centre.
At the point of contact with the ground, these velocities cancel instantaneously, giving
At the top of the wheel, the two velocity contributions act in the same direction, giving
Question: A wheel rolls without slipping with its centre moving at 6 m/s. Determine the instantaneous speeds of the highest point and the point in contact with the ground.
Solution:
Answer: The highest point moves at 12 m/s, while the contact point is instantaneously at rest relative to the ground.
10.13 Energy of a Rolling Body
A rolling body possesses translational kinetic energy because its centre of mass moves and rotational kinetic energy because it rotates about its centre of mass.
The total kinetic energy is therefore
For rolling without slipping,
Thus,
Question: A solid cylinder of mass 4 kg and radius 0.50 m rolls without slipping at 3 m/s. Find its total kinetic energy.
Moment of Inertia:
Angular Speed:
Translational Kinetic Energy:
Rotational Kinetic Energy:
Total:
Answer: The total kinetic energy is 27 J.
10.14 Rolling Down an Inclined Plane
Consider a rigid body of mass M and radius R rolling without slipping down an incline at angle θ.
The component of weight parallel to the slope is Mg sinθ. Static friction provides the torque required for angular acceleration.
For translation,
For rotation about the centre of mass,
Since pure rolling requires
we have
Substitution into the translational equation gives
Therefore,
This result shows that the acceleration depends on how the mass is distributed. Objects of the same mass and radius but different moments of inertia can therefore roll down the same incline with different accelerations.
Question: A uniform solid cylinder rolls without slipping down a plane inclined at 30° to the horizontal. Find its acceleration. Take g=9.8 m/s2.
For a Solid Cylinder:
Formula:
Substitution:
Answer: The acceleration is approximately 3.27 m/s2.
Energy Method for Rolling Bodies:
When dissipative forces are negligible, conservation of mechanical energy provides another efficient method of analysing rolling motion.
If a body starts from rest at height h and rolls without slipping,
Using ω=v/R,
Question: A solid sphere rolls without slipping from rest through a vertical height of 5 m. Find its speed at the bottom. Take g=9.8 m/s2 and I=(2/5)MR2.
Conservation of Energy:
Using I=(2/5)MR2 and ω=v/R,
Answer: The sphere reaches the bottom with a speed of approximately 8.37 m/s.
10.15 Applications of Gyroscopic and Rotational Principles
The principles developed in this chapter occur in many physical and technological systems. Their usefulness follows from the relationships among torque, angular momentum, moment of inertia and rotational motion.
Spinning Tops:
A spinning top has angular momentum along its spin axis. Gravity produces a torque about the point of contact, causing the axis to precess. As friction gradually reduces the spin speed, the motion becomes less stable and the top eventually falls.
Bicycles and Motorcycles:
Rotating wheels possess angular momentum. Gyroscopic effects can contribute to the dynamics of steering and stability, although real bicycle stability also depends on steering geometry, speed, mass distribution and rider control. It is therefore inaccurate to attribute bicycle stability to gyroscopic action alone.
Navigation and Orientation:
Gyroscopic devices can provide information about orientation and angular motion. Modern inertial systems commonly use compact mechanical or electronic angular-rate sensors based on gyroscopic principles.
Flywheels:
A flywheel stores rotational kinetic energy:
A large moment of inertia and high angular speed allow significant energy storage. Flywheels can also help smooth variations in the rotational speed of machinery.
Question: A flywheel has moment of inertia 20 kg m2 and rotates at 50 rad/s. Find the rotational kinetic energy stored.
Formula:
Solution:
Answer: The flywheel stores 25,000 J, or 25 kJ, of rotational kinetic energy.
Rotational Power in Machines:
For a rotating shaft transmitting torque τ at angular speed ω, mechanical power is
Question: A motor delivers a torque of 40 N m while its shaft rotates at 25 rad/s. Determine its mechanical power output.
Formula:
Solution:
Answer: The mechanical power output is 1000 W = 1.0 kW.
Gyroscopic motion is not a separate set of laws. It follows directly from Newtonian rotational mechanics. Torque changes angular momentum, conservation of angular momentum governs isolated rotating systems, and moment of inertia determines how mass distribution influences rotational response.
Chapter Summary
- A gyroscope is a rapidly spinning body whose axis is free to change direction.
- For rotation about a fixed principal axis, angular momentum is L=Iω.
- External torque changes angular momentum according to Στext=dL/dt.
- A large angular momentum makes a rapidly spinning body's orientation comparatively resistant to rapid change.
- Precession is the relatively slow rotation of a spinning body's axis under an applied torque.
- For a rapidly spinning gyroscope undergoing steady precession with a horizontal axle under gravity, Ω=Mgl/(Iω).
- Nutation is an oscillatory variation in the inclination of a spinning body's axis that may accompany precession.
- When external torque is zero, total angular momentum remains constant.
- Angular momentum may be conserved even when mechanical energy is not conserved.
- Rolling motion combines translation of the centre of mass and rotation about the centre of mass.
- For pure rolling without slipping, vcm=Rω.
- The total kinetic energy of a rolling body is the sum of translational and rotational kinetic energies.
- The acceleration of a body rolling down an incline depends on its moment of inertia and therefore on its mass distribution.
- Gyroscopic and rotational principles have applications in rotating machinery, flywheels, navigation, vehicles and many other mechanical systems.
CHAPTER ELEVEN
Gravitation and Motion Under Gravity
11.1 Introduction to Gravitation
Gravitation is one of the fundamental interactions of nature and is responsible for many familiar phenomena: objects fall toward the Earth, the Moon remains associated with the Earth, planets move around the Sun, and large astronomical structures are held together by mutual attraction.
In elementary mechanics, gravity is often introduced as a nearly constant downward force near the Earth's surface. A more complete treatment shows that this familiar force is one manifestation of a universal interaction between masses.
Gravitation is the mutual attractive interaction between bodies that possess mass.
Newton's law of universal gravitation gives the quantitative relationship governing this attraction in classical mechanics.
11.2 Newton's Law of Universal Gravitation
Every two point masses attract each other with a force directly proportional to the product of their masses and inversely proportional to the square of the distance between them.
If two point masses m1 and m2 are separated by a distance r, then the magnitude of the gravitational force is
The force acts along the line joining the two masses. Each mass exerts a force of equal magnitude and opposite direction on the other, in agreement with Newton's third law.
If the separation between two masses is doubled, the gravitational force becomes one-quarter of its original value. If the separation is tripled, the force becomes one-ninth.
Question: Two masses of 5 kg and 8 kg are separated by 2 m. Calculate the gravitational force between them. Take G=6.67×10-11 N m2/kg2.
Given:
Formula:
Solution:
Answer: The gravitational attraction is 6.67×10-10 N.
11.3 Gravitational Constant
The constant G in Newton's gravitational law is called the universal gravitational constant.
Its dimensions may be determined from
Therefore,
Question: State the SI unit and dimensions of the universal gravitational constant.
Answer: SI unit: N m2/kg2; dimensions: M-1L3T-2.
11.4 Gravitational Field and Field Strength
A gravitational field is a region of space in which a mass experiences gravitational force.
The gravitational field strength at a point is the gravitational force per unit mass experienced by a small test mass placed at that point.
For a point mass M, the magnitude of the field strength at distance r is
Its direction is toward the attracting mass.
The SI unit of gravitational field strength is
which is equivalent to
Question: Calculate the gravitational field strength at a distance of 7.0×106 m from the centre of a planet of mass 6.0×1024 kg.
Formula:
Solution:
Answer: The gravitational field strength is approximately 8.17 N/kg, directed toward the planet.
11.5 Acceleration Due to Gravity
A freely falling body near the Earth's surface accelerates because of the Earth's gravitational field. Ignoring air resistance, the acceleration is independent of the mass of the falling body.
If the Earth has mass ME and radius RE, then at the surface
Near sea level, a commonly used approximate value is
In many introductory calculations, g=9.8m/s2 or 9.81m/s2 is used unless another value is specified.
Question: Estimate the acceleration due to gravity at the Earth's surface using ME=5.97×1024 kg, RE=6.37×106 m, and G=6.67×10-11 N m2/kg2.
Formula:
Solution:
Answer: The calculated value is approximately 9.81 m/s2.
11.6 Variation of Gravitational Acceleration with Altitude
At height h above the Earth's surface, the distance from the Earth's centre is
Therefore,
Since at the surface
we may write
Thus gravitational acceleration decreases as altitude increases.
Question: At what height above a planet's surface would the gravitational acceleration become one-quarter of its surface value, assuming the planet has radius R?
Given:
Formula:
Solution:
Taking positive square roots,
Answer: The height is equal to one planetary radius.
11.7 Variation of Gravitational Acceleration with Depth
A simplified treatment is possible if the Earth is modelled as a sphere of uniform density. At a distance r from the centre, only the mass enclosed within radius r contributes to the net gravitational force.
For uniform density,
Hence,
Since g=GM/R2 at the surface,
If depth below the surface is d, then r=R-d, so
The linear relation with depth assumes uniform density. The real Earth is not of uniform density, so the actual variation is more complicated.
Question: In a uniform spherical planet, determine the gravitational acceleration at a depth equal to one-quarter of the planetary radius.
Given:
Formula:
Solution:
Answer: The gravitational acceleration is 0.75g.
11.8 Gravitational Potential
The gravitational potential at a point is the gravitational potential energy per unit mass of a small test mass placed at that point.
Taking gravitational potential to be zero at infinity, the potential due to a point mass M at distance r is
The SI unit of gravitational potential is joule per kilogram,
The negative sign reflects the choice of zero potential at infinity and the attractive nature of gravitational interaction.
Question: Calculate the gravitational potential at a point 4×106 m from the centre of a planet of mass 2×1024 kg.
Formula:
Solution:
Answer: The gravitational potential is approximately -3.34×107 J/kg.
11.9 Gravitational Potential Energy
If a mass m is placed in a gravitational potential V, its potential energy is
Therefore, for two point masses M and m separated by distance r,
This expression is more general than the near-surface approximation U=mgh. The approximation mgh is useful only when the change in height is small compared with the Earth's radius and g can be regarded as constant.
Question: A 100 kg object is at a distance of 8×106 m from the centre of a planet of mass 6×1024 kg. Find its gravitational potential energy.
Formula:
Solution:
Answer: The gravitational potential energy is approximately -5.00×109 J.
11.10 Relationship Between Field Strength and Potential
Gravitational field strength and gravitational potential are related. In radial motion,
More generally,
The negative sign means that the gravitational field points in the direction in which potential decreases most rapidly.
For
we obtain
Therefore,
where the negative radial sign indicates that the field points inward toward the mass.
11.11 Free Fall
Free fall is motion in which gravity is the only force acting on a body.
Near the Earth's surface, neglecting air resistance, free-fall motion has approximately constant downward acceleration g.
If downward is chosen as positive and a body is released from rest,
The equations of motion become
and
Question: A stone is dropped from rest and falls freely for 3 s. Find its speed and distance fallen. Take g=9.8 m/s2.
Speed:
Distance:
Answer: Speed = 29.4 m/s downward; distance fallen = 44.1 m.
Question: A stone is dropped from a height of 78.4 m. How long does it take to reach the ground, neglecting air resistance?
Formula:
Solution:
Answer: The stone reaches the ground after 4 s.
11.12 Vertically Projected Bodies
Consider an object projected vertically upward with initial speed u. If upward is chosen as positive, gravitational acceleration is
The velocity after time t is
The displacement is
Also,
Maximum Height:
At the highest point, the instantaneous velocity is zero:
Thus,
Therefore,
Time to Reach Maximum Height:
Using v=u-gt and setting v=0,
Total Time of Flight:
If the object returns to its point of projection and air resistance is neglected,
Question: A ball is thrown vertically upward at 19.6 m/s. Find the time to reach maximum height, maximum height, and total time to return to the point of projection. Take g=9.8 m/s2.
Time to Maximum Height:
Maximum Height:
Total Time:
Answer: Time to maximum height = 2 s; maximum height = 19.6 m; total time of flight = 4 s.
Question: A ball is projected vertically upward at 30 m/s. Find its velocity after 2 s. Take upward as positive and g=9.8 m/s2.
Formula:
Solution:
Answer: The ball is still moving upward at 10.4 m/s.
11.13 Motion Downward Under Gravity
A body may also be projected downward with an initial velocity. If downward is chosen as positive, then
The equations are
and
Question: A stone is thrown vertically downward at 5 m/s from a height of 40 m. Find its speed just before reaching the ground. Take g=9.8 m/s2.
Given:
Formula:
Solution:
Answer: The speed just before impact is approximately 28.44 m/s.
11.14 Weightlessness and Free-Fall Frames
A person may experience apparent weightlessness when both the person and the supporting environment are accelerating freely under gravity.
A weighing scale measures normal reaction rather than gravitational force directly. During ideal free fall,
The person still experiences gravitational attraction, but there is no supporting normal force. Apparent weightlessness therefore does not mean the absence of gravity.
Astronauts in an orbiting spacecraft appear weightless because both the spacecraft and the astronauts are continuously falling under gravity together. Their orbital motion prevents them from striking the Earth's surface.
11.15 Applications of Motion Under Gravity
The principles of motion under gravity apply to falling bodies, vertically launched objects, projectiles, planetary motion and satellite motion. Careful choice of sign convention is essential.
Question: A ball is thrown vertically upward from the top of a 30 m building with speed 14 m/s. Find the maximum height above the ground. Take g=9.8 m/s2.
Additional Height Above the Building:
Total Height Above Ground:
Answer: The maximum height above the ground is 40 m.
Question: An object falls freely from rest. Determine its speed after falling 20 m. Take g=9.8 m/s2.
Formula:
Solution:
Answer: The speed is approximately 19.8 m/s downward.
Chapter Summary
- Gravitation is the mutual attractive interaction between masses.
- Newton's law of universal gravitation is F=Gm1m2/r2.
- The universal gravitational constant is approximately 6.67×10-11 N m2/kg2.
- Gravitational field strength is force per unit mass.
- For a point or spherical mass, g=GM/r2.
- At the surface of a spherical planet, g=GM/R2.
- Gravitational acceleration decreases with increasing altitude.
- For a uniform spherical planet, gravitational acceleration decreases linearly with depth below the surface.
- Taking zero potential at infinity, gravitational potential is V=-GM/r.
- Gravitational potential energy is U=-GMm/r.
- The gravitational field is related to potential through g=-∇V.
- Free fall is motion under gravity alone.
- Near the Earth's surface, free-fall motion can be treated using constant acceleration g.
- For vertical upward projection, maximum height is H=u2/(2g) and time to maximum height is u/g.
- Apparent weightlessness occurs when the normal supporting force becomes zero during free fall.
CHAPTER TWELVE
Planetary Motion, Satellites and Escape Velocity
12.1 Introduction to Planetary Motion
The motions of planets and satellites provide some of the most important applications of Newtonian mechanics. The same laws that describe falling objects and circular motion near the Earth's surface can also explain the motion of planets around the Sun and satellites around planets.
Before Newton formulated the universal law of gravitation, Johannes Kepler summarized planetary observations in three empirical laws. Newton later showed that these laws follow naturally from gravitational attraction and the laws of motion.
12.2 Kepler's First Law
Every planet moves in an elliptical orbit with the Sun located at one focus of the ellipse.
A circle is a special case of an ellipse. Many planetary orbits have relatively small eccentricities and may appear nearly circular, but their exact classical form is elliptical.
The point of closest approach of a planet to the Sun is called perihelion, while the farthest point is called aphelion.
12.3 Kepler's Second Law
The line joining a planet to the Sun sweeps out equal areas in equal intervals of time.
This law implies that a planet moves faster when it is closer to the Sun and slower when it is farther away.
The law is closely connected with conservation of angular momentum. For a central gravitational force,
because the gravitational force is directed along the radius vector. Therefore,
and angular momentum is conserved.
Kepler's second law is a geometrical expression of angular momentum conservation for motion under a central force.
12.4 Kepler's Third Law
For bodies orbiting the same central mass, the square of the orbital period is proportional to the cube of the semi-major axis of the orbit.
For circular orbits, the semi-major axis is simply the orbital radius r, so
For two bodies orbiting the same central mass,
Question: Satellite B orbits the same planet as Satellite A at four times A's orbital radius. If A's period is 2 h, find B's orbital period.
Formula:
Given:
Solution:
Answer: Satellite B has an orbital period of 16 h.
12.5 Newtonian Interpretation of Kepler's Laws
Newton showed that planetary motion can be understood from the inverse-square gravitational force
For a circular orbit, this gravitational force supplies exactly the required centripetal force:
This relationship leads directly to the expressions for orbital velocity and orbital period.
More generally, the inverse-square nature of gravity leads to conic-section trajectories, including circles, ellipses, parabolas and hyperbolas, depending on the total mechanical energy and initial conditions.
12.6 Circular Orbital Motion
A satellite in a circular orbit is continuously falling toward the central body. However, its tangential velocity carries it forward so that the curvature of its falling path matches the curvature of the orbit.
The gravitational force provides the centripetal force:
The satellite mass m cancels:
Thus orbital motion does not depend on the satellite's mass when other effects are neglected.
12.7 Orbital Velocity
From the circular orbit condition,
The orbital velocity of a body in a circular orbit is the tangential speed required for gravitational attraction to provide exactly the centripetal force needed to maintain that orbit.
As orbital radius increases, circular orbital speed decreases.
Question: Estimate the circular orbital speed of a satellite at a distance of 7.0×106 m from the centre of the Earth. Take G=6.67×10-11 and ME=5.97×1024 kg.
Formula:
Solution:
Answer: The orbital speed is approximately 7.54 km/s.
12.8 Orbital Period
For one complete circular orbit,
Substitute
Then
Therefore,
Squaring gives
which is the Newtonian form of Kepler's third law for circular orbits.
Question: A satellite moves in a circular orbit of radius 7.0×106 m around the Earth. Using GME≈3.986×1014 m3/s2, calculate its orbital period.
Formula:
Solution:
Converting to minutes,
Answer: The period is approximately 5.83×103 s, or 97.2 minutes.
12.9 Energy of a Satellite in Circular Orbit
A satellite in orbit possesses both kinetic energy and gravitational potential energy.
The gravitational potential energy is
For a circular orbit,
Therefore the kinetic energy is
The total mechanical energy is
Hence,
Thus the total energy of a satellite in a circular gravitational orbit is negative, indicating that the satellite is gravitationally bound.
Question: A 500 kg satellite moves in a circular orbit of radius 8.0×106 m around Earth. Take GME=3.986×1014 m3/s2. Find its total mechanical energy.
Formula:
Solution:
Answer: The total mechanical energy is approximately -1.25×1010 J.
12.10 Artificial Satellites
An artificial satellite is a human-made object intentionally placed into orbit around the Earth or another astronomical body.
Artificial satellites are used for communication, navigation, weather observation, scientific research, Earth observation and many other purposes.
The properties of a satellite orbit depend primarily on the central mass, orbital radius, orbital speed and orbital geometry.
Low-Earth Orbits:
Satellites in relatively low orbits have shorter periods and comparatively high orbital speeds. They may pass over different regions of the Earth as the Earth rotates beneath them.
Higher Orbits:
A satellite in a larger orbit moves more slowly and takes longer to complete one revolution, in accordance with Kepler's third law.
In orbital equations, r is measured from the centre of the Earth or other central body, not from its surface. If the altitude is h, then r=R+h.
12.11 Geostationary Satellites
A geostationary satellite is a satellite in a circular equatorial orbit that moves in the same rotational sense as the Earth and has an orbital period equal to the Earth's rotation period, so it appears fixed above one point on the equator.
For geostationary motion, the orbital period is approximately one sidereal day. Using
we can solve for the required orbital radius:
The required orbital radius is about 4.22×107 m from the Earth's centre, corresponding to an altitude of roughly 3.58×107 m, or about 35,800 km, above the equator.
Question: Explain why a geostationary satellite cannot orbit directly above the North Pole.
Answer: A geostationary satellite must remain above the same point on the Earth. This requires a circular orbit in the equatorial plane with the same angular speed and rotational direction as the Earth. An orbit above the poles does not remain fixed over a single surface point and is therefore not geostationary.
12.12 Escape Velocity
Escape velocity is the minimum initial speed required for an object to move away from a gravitational body and reach infinitely large distance with zero remaining speed, assuming no further propulsion and neglecting atmospheric resistance and other bodies.
Suppose a body of mass m is launched from a distance R from the centre of a planet of mass M.
Initial total energy is
For the minimum escape condition, the body reaches infinity with zero speed. At infinity,
By conservation of mechanical energy,
Hence,
Therefore,
Since g=GM/R2 at the surface,
Question: Estimate the escape velocity from the Earth's surface using g=9.8 m/s2 and R=6.37×106 m.
Formula:
Solution:
Answer: The escape velocity is approximately 11.2 km/s.
The mass of the escaping object cancels from the derivation. Therefore, in the idealized model, escape velocity does not depend on the mass of the escaping body.
12.13 Relationship Between Escape and Orbital Velocity
At the same distance r from a central mass, the circular orbital speed is
The escape speed is
Therefore,
Question: The circular orbital speed at a certain radius around a planet is 7.5 km/s. Find the escape speed from the same radius.
Formula:
Solution:
Answer: The escape speed is approximately 10.61 km/s.
12.14 Bound and Unbound Gravitational Motion
The total mechanical energy of a body in a gravitational field helps determine the nature of its motion.
| Total Mechanical Energy | Nature of Motion |
|---|---|
| E<0 | Bound gravitational orbit, such as a circle or ellipse. |
| E=0 | Threshold escape trajectory, corresponding ideally to a parabolic path. |
| E>0 | Unbound trajectory with excess speed at large distance, corresponding ideally to a hyperbolic path. |
For a circular orbit,
so a circularly orbiting satellite is gravitationally bound.
Question: A spacecraft at a certain point has kinetic energy 8×109 J and gravitational potential energy -1.1×1010 J. Determine whether it is gravitationally bound.
Formula:
Solution:
Answer: Since the total mechanical energy is negative, the spacecraft is gravitationally bound.
12.15 Applications of Satellite Motion
Artificial satellites are among the most important practical applications of gravitation and orbital mechanics. Their usefulness depends on selecting orbital properties suited to a particular purpose.
Communication:
Communication satellites relay signals between widely separated regions. Geostationary satellites are especially useful when a fixed apparent position in the sky is desirable for ground antennas.
Weather Observation:
Meteorological satellites observe cloud systems, atmospheric conditions and weather patterns. Different orbital configurations provide different combinations of coverage and observation frequency.
Navigation:
Satellite navigation systems use accurately known satellite positions and timing signals to enable receivers to determine location and time.
Earth Observation:
Remote-sensing satellites collect information about land, oceans, vegetation, natural hazards and environmental change.
Scientific Research:
Satellites and space probes are used to study the Earth, Sun, planets and the wider universe. Orbital mechanics determines how such spacecraft are launched, transferred between orbits and maintained in useful trajectories.
Question: A satellite is moved from a circular orbit of radius r to a larger circular orbit of radius 4r. Compare the new circular orbital speed with the original speed.
Formula:
Original speed:
New speed:
Answer: At four times the orbital radius, the circular orbital speed is half the original speed.
Question: A satellite in a circular orbit has period 3 h. Another satellite orbits the same planet at nine times the first satellite's orbital radius. Determine the second satellite's period.
Kepler's Third Law:
Answer: The second satellite has a period of 81 h.
Question: A satellite has circular orbital speed 8 km/s. If its orbital radius is doubled while it remains in a circular orbit around the same planet, determine its new speed.
Relationship:
Therefore,
Answer: The new circular orbital speed is approximately 5.66 km/s.
Planetary and satellite motion brings together the major ideas developed throughout mechanics: vectors, kinematics, Newton's laws, circular motion, work and energy, conservation principles and gravitation. The same fundamental laws describe both ordinary terrestrial motion and the large-scale motion of astronomical bodies.
Chapter Summary
- Kepler's first law states that planetary orbits are ellipses with the Sun at one focus.
- Kepler's second law states that the line joining a planet to the Sun sweeps out equal areas in equal times.
- Kepler's second law is closely connected with conservation of angular momentum.
- Kepler's third law gives T2∝a3 for bodies orbiting the same central mass.
- For circular motion under gravity, gravitational force supplies the centripetal force.
- Circular orbital speed is v=√(GM/r).
- The circular orbital period is T=2π√(r3/GM).
- For a satellite in circular orbit, kinetic energy is GMm/(2r).
- Its gravitational potential energy is -GMm/r.
- Its total mechanical energy is -GMm/(2r).
- A geostationary satellite must orbit in the equatorial plane, in the direction of Earth's rotation, with the same angular period as the Earth's rotation.
- Escape velocity from radius R is ve=√(2GM/R).
- At the same radius, escape speed is √2 times the circular orbital speed.
- Negative total gravitational mechanical energy indicates a bound orbit.
- Zero or positive total gravitational energy corresponds to the threshold of escape or an unbound trajectory.
- Satellite mechanics has major applications in communication, navigation, meteorology, Earth observation and scientific research.
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