Topics
Units and Measurements
- Quantitative Science
- System of Units
- Derived Quantities and Units
- Rules and Conventions for Writing SI Units and Their Symbols
- Measurement of Length
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- Dimensions and Dimensional Analysis
- Accuracy, Precision and Uncertainty in Measurement
- Errors in Measurements>Systematic Errors
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- Estimation of Errors
- Combination of Errors
- Significant Figures
- Definitions of SI Units and Constants
Mathematical Methods
- Vector Analysis
- Scalar
- Vector
- Vector Operations>Multiplication of a Vector by a Scalar
- Vector Operations>Addition and Subtraction of Vectors
- Vector Operations>Triangle Law for Vector Addition
- Vector Operations>Law of parallelogram of vectors
- Resolution of Vectors
- Multiplication of Vectors
- Scalar Product(Dot Product)
- Vector Product (Cross Product)
- Concept of Calculus
- Differential Calculus
- Integral Calculus
Motion in a Plane
- Concept of Motion
- Rectilinear Motion
- Displacement
- Path Length
- Average Velocity
- Average Speed
- Instantaneous Velocity
- Instantaneous Speed
- Acceleration in Linear Motion
- Relative Velocity
- Motion in Two Dimensions-Motion in a Plane
- Average and Instantaneous Velocities
- Acceleration in a Plane
- Equations of Motion in a Plane with Constant Acceleration
- Relative Velocity in Two Dimensions
- Projectile Motion
- Uniform Circular Motion (UCM)
- Key Parameters of Circular Motion
- Centripetal Acceleration
- Conical Pendulum
Laws of Motion
- Fundamental Principles of Motion and Mechanics
- Types of Motion
- Aristotle’s Fallacy
- Newton’s Laws of Motion
- Newton's First Law of Motion
- Newton’s Second Law of Motion
- Newton's Third Law of Motion
- Inertial and Non-inertial Frames of Reference
- Types of Forces>Fundamental Forces in Nature
- Types of Forces>Contact and Non-Contact Forces
- Types of Forces>Real and Pseudo Forces
- Types of Forces>Conservative and Non-Conservative Forces
- Types of Forces>Work Done by a Variable Force
- Work Energy Theorem
- Principle of Conservation of Linear Momentum
- Collisions
- Elastic and Inelastic Collisions
- Perfectly Inelastic Collision
- Coefficient of Restitution e
- Expressions for Final Velocities in Elastic Head-On Collision
- Loss of Kinetic Energy in Perfectly Inelastic Head-On Collision
- Collision in Two Dimensions
- Impulse of a Force
- Necessity of Defining Impulse
- Rotational Analogue of a Force: Moment of a Force Or Torque
- Couple and Its Torque
- Proof of Independence of the Axis of Rotation
- Mechanical Equilibrium
- States of Equilibrium
- Centre of Mass>Mathematical Understanding of Centre of Mass
- Centre of Mass>Velocity of Centre of Mass
- Centre of Mass>Acceleration of Centre of Mass
- Centre of Mass>Characteristics of Centre of Mass
- Centre of Gravity
Gravitation
- Concept of Gravitation
- Kepler’s Laws
- Law of Orbit or Kepler's First Law
- Law of Areas or Kepler's Second Law
- Law of Periods or Kepler's Third Law
- Newton's Universal Law of Gravitation
- Measurement of the Gravitational Constant (G)
- Acceleration Due to Gravity (Earth’s Gravitational Acceleration)
- Variation in the Acceleration>Variation in Gravity with Altitude
- Variation in the Acceleration>Variation in Gravity with Depth
- Variation in the Acceleration>Variation in Gravity with Latitude and Rotation of the Earth
- Variation in the Acceleration>Effect of the shape of the Earth
- Gravitational Potential Energy
- Expression for Gravitational Potential Energy
- Connection of Potential Energy Formula with mgh
- Potential and Potential Difference
- Escape Velocity
- Earth Satellites
- Projection of Satellite
- Weightlessness in a Satellite
- Time Period of Satellite
- Binding Energy of an Orbiting Satellite
Mechanical Properties of Solids
- Mechanical Properties of Solids
- Elastic Behavior of Solids
- Stress and Strain
- Types of Stress and Corresponding Strain
- Hooke’s Law
- Elastic Modulus>Young’s Modulus
- Elastic Modulus>Bulk Modulus
- Elastic Modulus>Modulus of Rigidity
- Elastic Modulus>Poisson’s Ratio
- Stress-strain Curve
- Strain Energy
- Hardness of Material
- Friction in Solids
- Origin of Friction
- Types of Friction>Static Friction
- Types of Friction>Kinetic Friction
- Types of Friction>Rolling Friction
Thermal Properties of Matter
- Thermal Properties of Matter
- Temperature and Heat
- Measurement of Temperature
- Absolute Zero and Absolute Temperature
- Ideal Gas Equation
- Thermal Expansion
- Linear Expansion
- Areal Expansion
- Volume Expansion
- Relation Between Coefficient of Expansion
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- Heat Equation
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- Calorimetry
- Change of State
- Analysis of Observation>From Point A to B
- Analysis of Observation>From Point B to D
- Temperature Effects and Considerations
- Evaporation vs Boiling
- Boiling Point and Pressure
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- Coefficient of Thermal Conductivity
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- Convection
- Application of Convection
- Free and Forced Convection
- Radiation
- Newton’s Law of Cooling
Sound
- Sound Waves
- Common Properties of All Waves
- Transverse Waves
- Longitudinal Waves
- Mathematical Expression of a Wave
- The Speed of Travelling Waves
- The Speed of Transverse Waves
- The Speed of Longitudinal Waves
- Newton's Formula for Velocity of Sound
- Laplace’s Correction
- Factors Affecting Speed of Sound
- Principle of Superposition of Waves
- Echo
- Reverberation
- Acoustics
- Qualities of Sound
- Doppler Effect
- Source Moving and Listener Stationary
- Listener Approaching a Stationary Source with Velocity
- Both Source and Listener are Moving
- Common Properties between Doppler Effect of Sound and Light
- Major Differences between Doppler Effects of Sound and Light
Optics
- Fundamental Concepts of Light
- Nature of Light
- Ray Optics Or Geometrical Optics
- Cartesian Sign Convention
- Reflection>Reflection from a Plane Surface
- Reflection>Reflection from Curved Mirrors
- Total Internal Reflection
- Refraction of Light
- Applications of Total Internal Reflection
- Refraction at a Spherical Surface and Lenses
- Thin Lenses and Their Combination
- Refraction at a Single Spherical Surface
- Lens Makers' Equation
- Dispersion of Light
- Analysis of Prism
- Thin Prisms
- Some Natural Phenomena Due to Sunlight
- Defects of Lenses
- Optical Instruments
- Simple Microscope or a Reading Glass
- Compound Microscope
- Telescope
Electrostatics
- Concept of Electrostatics
- Electric Charge
- Basic Properties of Electric Charge
- Additive Nature of Charge
- Quantization of Charge
- Conservation of Charge
- Force between Charges
- Coulomb’s Law
- Scalar Form of Coulomb’s Law
- Relative Permittivity or Dielectric Constant
- Definition of Unit Charge from the Coulomb’s Law
- Coulomb's Law in Vector Form
- Principle of Superposition
- Electric Field
- Electric Field Intensity Due to a Point-Charge
- Practical Way of Calculating Electric Field
- Electric Lines of Force
- Electric Flux
- Gauss’s Law
- Electric Dipole
- Couple Acting on an Electric Dipole in a Uniform Electric Field
- Electric Intensity at a Point Due to an Electric Dipole
- Continuous Charge Distribution
Electric Current Through Conductors
- Concept of Electric Currents in Conductors
- Electric Current
- Flow of Current Through a Conductor
- Drift Speed
- Ohm's Law
- Limitations of Ohm’s Law
- Electrical Power
- Resistors
- Rheostat
- A combination of resistors in both series and parallel
- Specific Resistance
- Variation of Resistance with Temperature
- Electromotive Force (emf)
- Cells in Series
- Cells in Parallel
- Types of Cells
Magnetism
- Concept of Magnetism
- Magnetic Lines of Force
- The Bar Magnet
- Magnetic Field due to a Bar Magnet
- Magnetic Field Due to a Bar Magnet at an Arbitrary Point
- Gauss' Law of Magnetism
- The Earth’s Magnetism
Electromagnetic Waves and Communication System
- Foundations of Electromagnetic Theory
- EM Wave
- Sources of EM Waves
- Characteristics of EM Waves
- Electromagnetic Spectrum
- Radio Waves
- Microwaves
- Infrared waves
- Visible Light
- Ultraviolet rays
- X-rays
- Gamma Rays
- Propagation of EM Waves
- Ground (surface) Wave
- Space wave
- Sky wave propagation
- Communication System
- Elements of a Communication System
- Commonly Used Terms in Electronic Communication System
- Modulation
Semiconductors
- Concept of Semiconductors
- Electrical Conduction in Solids
- Band Theory of Solids
- Intrinsic Semiconductor
- Extrinsic Semiconductor
- n-type semiconductor
- p-type semiconductor
- Charge neutrality of extrinsic semiconductors
- p-n Junction
- A p-n Junction Diode
- Basics of Semiconductor Devices
- Applications of Semiconductors and P-n Junction Diode
- Thermistor
- Introduction
- Definition: Critical Velocity
- Formula: Critical Velocity
- Understanding Critical Velocity
- Five Cases of Satellite Orbits
- Special Case
- Significance
- Example
Introduction
To launch an artificial satellite into orbit around Earth, we need to give it a specific horizontal velocity at a particular height. A satellite requires a minimum two-stage rocket because the first stage lifts it to the desired height, and the second stage gives it horizontal velocity. The exact horizontal velocity needed for a satellite to revolve in a stable circular orbit around Earth is called critical velocity or orbital velocity. This velocity depends on the height of the satellite and Earth's mass, not on the satellite's mass. Understanding critical velocity is essential for successful satellite deployment and mission planning.
Definition: Critical Velocity
The exact horizontal velocity of projection that must be given to a satellite at a certain height so that it can revolve in a circular orbit around the Earth is called the critical velocity or orbital velocity (vc).
Formula: Critical velocity
vc = \[\sqrt{\frac{GM}{R+h}}\]
Where:
- vc = critical velocity (m/s)
- G = gravitational constant (6.67 × 10⁻¹¹ N·m²/kg²)
- M = mass of the Earth (kg)
- R = radius of the Earth (km)
- h = height of satellite above Earth's surface (km)
Understanding Critical Velocity
The critical velocity is derived by equating the centripetal force (needed for circular motion) with the gravitational force (pulling the satellite toward Earth).
For a satellite to move in a stable circular orbit, the gravitational force must provide exactly the right amount of centripetal force. If the velocity is too low, the satellite will fall back to Earth. If it's too high, it will either enter an elliptical orbit or escape Earth's gravitational influence entirely.
Five Cases of Satellite Orbits:
Various possible orbits depending on the value of vh.
Case (I): vh < vc (Velocity Less Than Critical Velocity)
- The satellite follows an elliptical orbit with the point of projection as the apogee (farthest point from Earth).
- If the satellite enters Earth's atmosphere during this elliptical path, air resistance causes energy loss, and the satellite spirals down and crashes.
Case (II): vh = vc (Velocity Equal to Critical Velocity)
- The satellite moves in a stable, circular orbit around Earth.
- This is the ideal condition for maintaining a stable orbit.
Case (III): vc < vh < ve (Velocity Between Critical and Escape Velocity)
- The satellite follows an elliptical orbit with the point of projection as the perigee (point closest to Earth).
- The satellite remains in orbit but travels farther away at the apogee.
Case (IV): vh = ve (Velocity Equal to Escape Velocity)
- The satellite travels along a parabolic path.
- It escapes Earth's gravitational influence but never returns to the initial point of projection.
- Its speed becomes zero at infinity.
Case (V): vh > ve (Velocity Greater Than Escape Velocity)
- The satellite follows a hyperbolic path.
- It completely escapes Earth's gravitational influence.
Special case
Satellite Close to Earth's Surface
When a satellite revolves very close to Earth's surface, the height (h) is negligible compared to Earth's radius (R). Therefore, we can assume R >> h, so (R + h) ≈ R.
vc = \[\sqrt{\frac{GM}{R}}\]
Since g = \[\frac {GM}{R^2}\], we have GM = gR2
Therefore:
vc = \[\sqrt{\frac{gR^{2}}{R}}=\sqrt{gR}\] = 7.92 km/s
This is the maximum possible critical speed and is approximately 25 times faster than the fastest passenger aeroplanes.
Important Facts:
- Critical velocity is independent of the satellite's mass—it depends only on Earth's mass and the orbital height.
- Critical velocity decreases with an increase in the height of the satellite.
- At Earth's surface, the critical velocity is 7.92 km/s.
Significance
- Satellite Launch Planning: Critical velocity determines the exact speed required to place a satellite in a stable orbit at a specific altitude.
- Mission Success: Achieving the correct critical velocity is essential for satellite stability; incorrect velocity leads to orbit failure or satellite loss.
- Fuel Efficiency: Understanding critical velocity helps rocket engineers calculate the minimum fuel needed for orbital insertion.
- Orbit Predictability: Critical velocity allows mission planners to predict satellite paths and orbital periods accurately.
- Independence from Satellite Mass: The formula shows that critical velocity depends only on orbital height and Earth's properties, making it applicable to all satellites regardless of their size or mass.
- Safety Consideration: Knowledge of critical velocity helps avoid escape velocities unintentionally, which would cause satellite loss.
Example
Problem:
Show that the critical velocity of a body revolving in a circular orbit very close to the surface of a planet of radius R and mean density ρ is vc = 2R\[\sqrt{\frac{G\pi\rho}{3}}\]
Solution:
- Since the body is revolving very close to the planet's surface, height h = 0.
- Express mass (M) in terms of density (ρ):
Density ρ = \[\frac {M}{V}\] = \[\frac{M}{\frac{4}{3}\pi R^3}\]
Therefore, M = \[\frac {4}{3}\]πR3ρ - Write the critical velocity formula:
vc = \[\sqrt{\frac{GM}{R}}\] - Substitute the expression for M:
vc = \[\sqrt{\frac{G\cdot\frac{4}{3}\pi R^3\rho}{R}}\] - Simplify:
vc = \[\sqrt{\frac{4G\pi R^3\rho}{3R}}=\sqrt{\frac{4G\pi R^2\rho}{3}}\] - Final result:
vc = 2R\[\sqrt{\frac{G\pi\rho}{3}}\]
Note:
This expression is derived assuming the satellite is very close to the planet's surface and air resistance is neglected. In reality, atmospheric friction would affect the satellite's motion.

