Kepler’s Laws of Planetary Motion
1 - Law of Orbits:
Each planet moves around the Sun in an elliptical orbit with the Sun at one of the foci
2 - Law of area:
The radial vector sweeps equal areas in equal intervals of time
3 - Law of Period:
The ratio of the square of the time period of a planet to the cubic power of semi major axis is constant for all the planets in the solar system
Kepler’s First Law
1 - Law of Orbits:
Each planet moves around the Sun in an elliptical orbit with the Sun at one of the foci
Kepler’s Second Law
2 - Law of area:
The radial vector sweeps equal areas in equal intervals of time
Kepler’s Third Law
3 - Law of Period:
The ratio of the square of the time period of a planet to the cubic power of semi major axis is constant for all the planets in the solar system
Newton’s Law of Gravitation
the gravitational force between two masses is
directly proportional to product of masses
inversely proportional to the square of the distance between the masses
Plasticity
If a body does not regain it's original shape and size after removal of the deforming force it is called plastic, with plasticity being the property
Pascal’s Law
If the pressure in a liquid is changed at a particular point, the change is transmitted to the entire liquid without being diminished in magnitude
Ex: Hydraulic lift
Viscosity
The property of a fluid to oppose the relative motion between its layers
(Friction acting between layers of liquid causing objects to slow down)
Buoyancy
The upward force exerted by a fluid that opposes the weight of an immersed object in a fluid
AKA “Upthrust” or “buoyant force”
Law of Floatation
A body will float in a liquid if the wright of a liquid displaced by the immersed part of the body equals the weight of the body
Streamlined flow
Each particle of a liquid passing through a point moves along the same path with the same velocity as its predecessor
Terminal velocuty
Maximum constant velocity acquired by a body while falling freely through a viscous medium
Intermolecular forces
Force acting between molecules
Cohesive force
Force between like molecules holding the liquid together
Ex: Mercury
Adhesive Force
Liquid in contact with a solid
Ex: Water and glass, ink and paper
Surface Tension
The force per unit length acting perpendicular to the imaginary line drawn on the liquids surface that tends to pull along the line
Ex: Needle on cup of water
Ex: Brush inside water is spread out, pulled together when outside
Factors affecting the surface tension of a liquid
Contamination/impurities
Dissolved substances
Electrification
Temperature
Angle of contact between the solid and the liquid
The angle between the tangent to the liquid surface at the point of contact and the solid surface inside the liquid
Capillarity/Capillary Action
Rise or fall of a liquid in a narrow tube
Practical applications of capillarity
Absorption of ink by blotting paper
Oil rises in the cotton in an earthen lamp
Sap rises form roots of a plant to its roots and branches
Stefan Boltzmann Law
the total amount of heat radiated per second per unit area of a black body is directly proportional to the fourth power of its absolute temperature
Wien’s Law
The wavelength of maximum intensity of emission of a black body radiation is inversely proportional to the absolute temperature of the black body
Provost Theory of Heat Exchange
All bodies emit thermal radiation at all temperatures above absolute zero irrespective of the nature of the surroundings
Thermodynamic system
A collection of large numbers of particles (atoms and molecules) specified by certain parameters
Parameters:
Pressure (P)
Volume (V)
Temperature (T)
Examples of thermodynamic system
Thermodynamic system | Surrounding |
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Bucket of water | Open atmosphere |
Air molecules in the room | Outside air |
Fish in the sea | Sea of water |
Thermal equilibrium
At the same temperature which will not change over time
Zeroth Law of Thermodynamics
If two systems, A and B, are in thermal equilibrium with a third system, C, than A and B are in thermal equilibrium with each other
First Law of Thermodynamics
Change in internal energy of the system is equal to the heat supplied to the system minus the work done by the system on the surroundings
Internal energy of a thermodynamic system
Heat flows into the system | Internal energy increases |
---|---|
Heat flows out of the system | Internal energy decreases |
Work is done on the system | Internal energy increases |
Work is done by the system | Internal energy decreases |
Thermodynamics sign convention
Action | Sign |
---|---|
Gains heat | Q is positive |
Loses heat | Q is negative |
Work done ON the system | W is negative |
Work done BY the system | W is positive |
Specific Heat Capacity
Amount of heat energy required to raise the temperature of one kg of a substance by 1K or 1C by keeping the pressure constant
Isothermal process
The temperature remains constant but the pressure and volume of a thermodynamic system will change
Adiabatic process
Pressure, volume, temperature may change
Isobaric Process
Pressure is constant
Temperature, volume, internal energy is not
Reversible Process
If it’s possible to retrace the path in the opposite direction and have it pass through the same states as the initial, direct process
Conditions for Reversible Process
Process should have extremely slow rate
Remain in mechanical, thermal, and chemical equilibrium at all times with the surroundings
No dissipative forces (friction, viscosity, electrical resistance) should be present
Irreversible process
All natural processes
Heat Engine Parts
Hot Reservoir
supplies heat
Working substance
converts heat supplied into work
gas or water
Cold Reservoir/Sink
absorbs heat
Entropy
Measure of disorder
Postulates of kinetic theory of gases
All molecules of a gas are identical, elastic spheres
Molecules of different gases are different
Number of molecules in a gas is very large and average separation between them is larger than size of the gas molecules
Molecules are in a state of continuous random motion
Molecules collide with each other and walls of the container
Collisions are perfectly elastic - no loss of kinetic energy
Between collisions, molecules move with uniform velocity
Molecules do not exert any force of attraction/repulsion on each other except during collision
Do not have any potential energy, energy is wholly kinetic
Collisions are instantaneous
Obey Newton’s Law’s of Motion even though they move randomly
Free oscillation
Vibrates with frequency equal to the natural frequency of the oscillator
Ex:
vibration of a tuning fork
oscillation of a simple pendulum
Damped oscillations
If oscillator moves in a resistive medium, amplitude goes on decreasing and the energy of the oscillator is used to do work against resistive medium
Maintained oscillations
Energy is supplied by an external source, so the amplitude of the oscillation can be made constant
Forced oscillations
Oscillator driven by an external periodic agency to overcome damping
Resonance
Frequency of external periodic force (driving force) matches with the natural frequency of vibrating body so the oscillating body’s amplitude increases at each step and ends up with a large amplitude
Wave
The disturbance which carries energy and momentum from one point in space to another point in space without the transfer of the medium
Characteristics of Wave Motion
for the propagation of waves, the medium must have both inertia and elasticity which decided velocity of the wave in that medium
in a given medium, the velocity of a wave is constant wheras the constituent particles in that medium move with different velocities at different positions
Velocity is maximum at their mean position and zero at extreme positions
waves undergo reflections, refractions, interference, diffraction, and polarization
Mechanical Wav Motion and Its Types
Mechanical Wave - require a medium
Ex: sound waves, ripples on water
Non mechanical Wave - do not require any medium
Ex: Light waves, infra red waves
Transverse vs. Longitudinal Waves
Transverse | Longitudinal |
---|---|
Direction of vibration of particles of the mdeium is perpendicular to the direction of propogation of waves | Direction of vibration of particles of the medium is parallel to the direction of the propagation of waves |
The disturbances are in the form of crests and troughs | The disturbances are in the form of compressions and rarefactions |
Transverse waves are possible in elastic medium | Longitudinal waves are possible in all types of media (solid, liquid, gas) |
Characteristics of Progressive Waves
Particles in the medium vibrate about their mean position with the same amplitude
Phase of every particle ranges from 0 to 2π
No particle remains at rest permanently. During propagation, come to rest position only twice at the extreme points (π and 2π)
Transverse progressive waves are characterized by crests and troughs. Longitudinal waves are characterized by compressions and rarefactions
When the particles pass through the mean position they always move with the same maximum velocity
Displacement, velocity, acceleration of particles separated from each other by nλ
Where:
n = integer
λ = wavelength
Standing/Stationary Waves
Waves in a pattern
Progressive vs. Stationary Waves
Progressive | Stationary |
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Waves carry energy while propagating | Waves do not transport energy |