This document contains a presentation by Prof. Mukesh N. Tekwani on various topics related to gravitation and orbital mechanics. It includes definitions and explanations of Newton's laws of gravitation and motion, Kepler's laws, gravitational constant, acceleration due to gravity, critical velocity and orbital velocity of satellites, time period of satellites, binding energy, escape velocity, weightlessness, and variation of gravitational acceleration with altitude, depth, and latitude. Equations are derived for many of these topics. Examples and assignments involving calculations are also provided. The document serves to instruct students on fundamental concepts in gravitation, orbital mechanics, and related physics.
The document discusses Newton's realization that the force of gravity on Earth must come from Earth itself and must also be what keeps the Moon in orbit. It then explains Newton's third law and how it applies to gravitational forces between objects of different masses. The document also defines the universal law of gravitation, including how the gravitational force between two objects is proportional to their masses and inversely proportional to the square of the distance between them. It further discusses how to calculate gravitational forces and acceleration due to gravity at different locations and distances from Earth.
This is the NCERT CBSE syllabus ppt on the topic Gravitation. It will be helpful for students studying in that class and will enable them to understand better.
1) The document discusses concepts related to gravitation including acceleration due to gravity, escape velocity, orbital velocity, gravitational potential, and Kepler's laws of planetary motion.
2) It explains that gravitational force is independent of intervening medium and obeys Newton's third law. The gravitational field modifies space around material bodies.
3) Satellites can be natural or artificial, and examples are given for different types including geostationary and polar satellites. Requirements for geostationary satellites are outlined.
1. Forces cause objects to accelerate by either speeding them up, slowing them down, or changing their direction.
2. For an object to travel in a circular path, it must be accelerating towards the center of the circle. This acceleration is caused by a centripetal force directed towards the center.
3. Examples of centripetal forces include the normal force from a rollercoaster track keeping a cart moving in a circle and gravity keeping satellites in orbit around Earth.
Periodic motion repeats at regular time intervals. Examples include planetary orbits and clock hands. Oscillation involves to-and-fro motion about a mean position, like a pendulum swing. It is always periodic but periodic motion need not involve oscillation. The time for one full cycle is the period (T). Frequency (ν) is the number of cycles per second. Angular frequency (ω) relates frequency and period. Displacement variables describe the changing quantity in oscillations, like position or angle. Simple harmonic motion involves a restoring force proportional to displacement towards the equilibrium point, like a spring. It can be modeled by sine and cosine functions and includes oscillations of springs and pendulums.
Introduction to Special theory of relativityROHIT PANJABI
This document provides an introduction to Einstein's special theory of relativity. It discusses key concepts like Galilean transformations, Michelson-Morley experiment, postulates of relativity, and consequences like time dilation and length contraction. The document explains that special relativity applies to observers in uniform motion and the speed of light in a vacuum is the same for all observers, regardless of their motion. It also presents the Lorentz transformations and equations for time dilation and length contraction.
Einstein’s Theories of Relativity revolutionized how Today’s Scientific world thinks about Space, Time, Mass, Energy and Gravity. This is purely an imaginative Science that worked in the Laboratory of Einstein's Brain..
1. The document defines key terms related to rotational motion such as angular position, angular displacement, angular velocity, and angular acceleration.
2. It also outlines the four fundamental equations of angular motion and how they are analogous to the linear equations of motion.
3. Key concepts such as moment of inertia, torque, angular momentum, and their relationships to linear motion are summarized.
The document discusses Newton's realization that the force of gravity on Earth must come from Earth itself and must also be what keeps the Moon in orbit. It then explains Newton's third law and how it applies to gravitational forces between objects of different masses. The document also defines the universal law of gravitation, including how the gravitational force between two objects is proportional to their masses and inversely proportional to the square of the distance between them. It further discusses how to calculate gravitational forces and acceleration due to gravity at different locations and distances from Earth.
This is the NCERT CBSE syllabus ppt on the topic Gravitation. It will be helpful for students studying in that class and will enable them to understand better.
1) The document discusses concepts related to gravitation including acceleration due to gravity, escape velocity, orbital velocity, gravitational potential, and Kepler's laws of planetary motion.
2) It explains that gravitational force is independent of intervening medium and obeys Newton's third law. The gravitational field modifies space around material bodies.
3) Satellites can be natural or artificial, and examples are given for different types including geostationary and polar satellites. Requirements for geostationary satellites are outlined.
1. Forces cause objects to accelerate by either speeding them up, slowing them down, or changing their direction.
2. For an object to travel in a circular path, it must be accelerating towards the center of the circle. This acceleration is caused by a centripetal force directed towards the center.
3. Examples of centripetal forces include the normal force from a rollercoaster track keeping a cart moving in a circle and gravity keeping satellites in orbit around Earth.
Periodic motion repeats at regular time intervals. Examples include planetary orbits and clock hands. Oscillation involves to-and-fro motion about a mean position, like a pendulum swing. It is always periodic but periodic motion need not involve oscillation. The time for one full cycle is the period (T). Frequency (ν) is the number of cycles per second. Angular frequency (ω) relates frequency and period. Displacement variables describe the changing quantity in oscillations, like position or angle. Simple harmonic motion involves a restoring force proportional to displacement towards the equilibrium point, like a spring. It can be modeled by sine and cosine functions and includes oscillations of springs and pendulums.
Introduction to Special theory of relativityROHIT PANJABI
This document provides an introduction to Einstein's special theory of relativity. It discusses key concepts like Galilean transformations, Michelson-Morley experiment, postulates of relativity, and consequences like time dilation and length contraction. The document explains that special relativity applies to observers in uniform motion and the speed of light in a vacuum is the same for all observers, regardless of their motion. It also presents the Lorentz transformations and equations for time dilation and length contraction.
Einstein’s Theories of Relativity revolutionized how Today’s Scientific world thinks about Space, Time, Mass, Energy and Gravity. This is purely an imaginative Science that worked in the Laboratory of Einstein's Brain..
1. The document defines key terms related to rotational motion such as angular position, angular displacement, angular velocity, and angular acceleration.
2. It also outlines the four fundamental equations of angular motion and how they are analogous to the linear equations of motion.
3. Key concepts such as moment of inertia, torque, angular momentum, and their relationships to linear motion are summarized.
This document discusses mass, weight, and density. It defines mass as a measure of the amount of substance in a body and explains that mass stays constant regardless of location, while weight depends on gravitational field strength and can vary in different locations. The document describes how gravitational field is a region where mass experiences gravitational force and how weight is calculated from mass and gravitational field strength. It provides equations for density and explains methods for measuring mass, weight, and density of liquids, regular solids, and irregular solids using balances and the displacement method.
This document discusses the universal law of gravitation and its implications. It can be summarized as follows:
1) The universal law of gravitation states that the gravitational force between two objects is directly proportional to the product of their masses and inversely proportional to the square of the distance between them.
2) This law explains phenomena like the orbit of planets around the sun and the moon around Earth. It also explains why objects fall with an acceleration of 9.8 m/s^2 on Earth.
3) The weight of an object, which is the gravitational force exerted by Earth, differs on other celestial bodies due to differences in their masses and radii. Calculations show an object's weight on
Here are the key steps to calculate the mass of Earth (M) from the given data:
1) Acceleration due to gravity on Earth's surface (g) = 9.81 m/s^2
2) Universal gravitational constant (G) = 6.67x10^-11 Nm^2/kg^2
3) Radius of Earth (R) = 6.37x10^6 m
4) Using the formula for acceleration due to gravity:
g = GM/R^2
5) Rearranging the terms:
M = gR^2/G
6) Substituting the values:
M = (9.81 m/s^2)(
Work is done when a force causes an object to be displaced. Work (W) is equal to force (F) multiplied by displacement (s). Work units are joules. Potential energy is stored energy due to an object's position or state. Kinetic energy is the energy of motion and depends on an object's mass and velocity. Power is the rate at which work is done or energy is converted and is measured in watts. Conservation of energy states that energy cannot be created or destroyed, only changed from one form to another.
Karen Adelan presented on the topic of classical mechanics and energy. Some key points:
- Energy is a conserved quantity that can change forms but is never created or destroyed. It is useful for describing motion when Newton's laws are difficult to apply.
- Kinetic energy is the energy of motion and depends on an object's mass and speed. The work-kinetic energy theorem states that the net work done on an object equals the change in its kinetic energy.
- Potential energy is the energy an object possesses due to its position or state. The work done by a constant force equals the product of force, displacement, and the cosine of the angle between them.
posted by Shifat Sanchez..</br>
its about relativity</BR.about sir albert Einstein. quotes about relativity...michelsone and morleys law about relativity....general theory of relativity ..Einstein laws about relativity...Einstein description of laws about theory of special relativity ....first postulates of special law,,sceond postulates of special laws of relativity.........Galilian transformation of relativity....................Lorentz transformation.......... Lorentz transformation about the laws of relativity........Length contractiion .....Time dilation........Mass expansion........E= MC^2 ( theory & provens ))......The life cycle of stars.......Black holes ( slides).............Formation And Properties of blackholes ................Concluation .........Thankyou slide ...............ANY QUESATION ?????????................thank YOU SO MUCH :P :P :P
* Mass of earth (M) = 5.98 x 1024 kg
* Radius of earth (R) = 6378100 m
* Gravitational constant (G) = 6.6726 x 10-11 N-m2/kg2
* Escape velocity (v) = √(2GM/R)
= √(2 x 6.6726 x 10-11 x 5.98 x 1024 / 6378100)
= √(2 x 3.986 x 1014 / 6378100)
= √(2 x 6.273 x 107)
= √1.2546 x 108
= 11.186 km/s
Therefore, the escape
this is class 12 Maharashtra board physics subject content. this is complete content with notes with easily explaination.
for buying or neet attractive ppt in any subject contact me 8879919898. go to my site akchem.tk
blog akchem.blogspot.com
The document discusses concepts related to mechanical energy, including work, kinetic energy, potential energy, and power. It defines energy as the capacity to do work and describes several forms of energy. Work is defined as the dot product of force and displacement. Kinetic energy is defined as 1/2mv^2 and depends on an object's motion. Potential energy exists in gravitational and elastic forms and depends on an object's position or state. The conservation of mechanical energy and work-energy theorem are explained. Power is defined as the rate of energy transfer.
The document discusses collisions and the law of conservation of momentum. It provides examples of how to use a momentum table and algebra to solve for unknown velocities in collision problems involving isolated systems where momentum is conserved. Specifically, it works through examples of a person catching a medicine ball on ice and of two people colliding on an ice rink to determine their combined velocity after collision.
Free fall is the downward motion of objects under the influence of gravity alone. All objects in free fall accelerate at the same rate of 9.8 m/s2 regardless of mass. Experiments show that free-falling objects do not encounter air resistance and accelerate constantly at 9.8 m/s2. Applications of free fall include skydiving and parachuting.
Parallax is the apparent change in position of an object when viewed from different positions. It can be used to measure distances to celestial objects. Stellar parallax involves measuring the difference in the position of a nearby star observed from opposite sides of Earth's orbit around the Sun. This allows astronomers to determine the star's distance using trigonometry. In 1989, the Hipparcos satellite improved parallax measurements for over 100,000 nearby stars. The Gaia satellite, launched in 2013, can measure parallax angles to greater accuracy, mapping stars up to tens of thousands of light years away.
The document discusses several topics related to heat and temperature, including:
1. It defines temperature as a measure of the average kinetic energy of atoms and molecules in a gas or substance, with higher temperatures corresponding to faster molecular motion.
2. It describes different devices that can be used to measure temperature, such as mercury thermometers, gas thermometers, pyrometers, and electrical resistance thermometers.
3. It explains concepts such as heat capacity, specific heat capacity, calorimetry, latent heat, phase changes, conduction, convection, radiation, and Newton's Law of Cooling.
Electric Charge and Electric Field LectureFroyd Wess
More: http://www.pinoybix.org
Lesson Objectives:
Static Electricity; Electric Charge and Its Conservation
Electric Charge in the Atom
Insulators and Conductors
Induced Charge; the Electroscope
Coulomb’s Law
Solving Problems Involving Coulomb’s Law and Vectors
The Electric Field
Field Lines
Electric Fields and Conductors
Gauss’s Law
Electric Forces in Molecular Biology: DNA Structure and Replication
Photocopy Machines and Computer Printers Use Electrostatics
Physics Project On Physical World, Units and MeasurementSamiran Ghosh
This PowerPoint is Physical World, Units and Measurement. This is basically the first chapter of 11th class/grade. This power point explains the basic or fundamental physics with some information about SI units and fundamental forces.
This document introduces the topic of electrostatics and electric charges and fields. Some key points include:
- Electrostatics deals with static electric charges and the forces, fields, and potentials arising from them. Charges can be positive or negative.
- The electric field is a vector quantity that describes the force exerted on a charge in a given point in space. It is calculated using Coulomb's law and the superposition principle.
- Electric field lines are imaginary lines used to depict electric fields graphically. They originate on positive charges and terminate on negative charges.
- Gauss's law relates the electric flux through a closed surface to the net charge enclosed by the surface. It can be used to calculate electric
The document provides information about current, electromotive force, potential difference, and resistance. It defines key terms, provides equations, and examples of calculations. It describes:
- Current is the flow of charge measured in amperes. It is carried by the flow of electrons in a conductor.
- Electromotive force is the work done per unit charge to drive charge around a complete circuit. It is measured in volts.
- Potential difference is the work done per unit charge to move charge through a circuit component. It is also measured in volts.
- Resistance is the opposition to current flow. It is calculated as potential difference divided by current and measured in ohms.
The center of mass of an object is the single point where the entire mass of the object is considered to be concentrated and acts as if the whole mass were located; it is defined mathematically as the weighted average of every discrete point making up the object. The document discusses center of mass for different geometric objects like cylinders, spheres, and distributed point masses, and explains that finding the center of mass allows predicting the object's motion as if all its mass were concentrated at that point.
Digital Library of GLT Saraswati Bal Mandir. Gravitation is a natural phenomenon by which all physical bodies attract each other. It is most commonly experienced as the agent that gives weight to objects with mass and causes them to fall to the ground when dropped.
Gravitation has been the most common phenomenon in our lives but somewhere down the line we don't know musch about it. So here is a presentation whic will help you out to know what it is !! I'll be makin it available for download once i submit it in school :P :P ! Coz last one of the brats showed the same presentation that i uploade and unfortunatele his roll number fell before mine ! I was damned..:D :D :P
This document discusses mass, weight, and density. It defines mass as a measure of the amount of substance in a body and explains that mass stays constant regardless of location, while weight depends on gravitational field strength and can vary in different locations. The document describes how gravitational field is a region where mass experiences gravitational force and how weight is calculated from mass and gravitational field strength. It provides equations for density and explains methods for measuring mass, weight, and density of liquids, regular solids, and irregular solids using balances and the displacement method.
This document discusses the universal law of gravitation and its implications. It can be summarized as follows:
1) The universal law of gravitation states that the gravitational force between two objects is directly proportional to the product of their masses and inversely proportional to the square of the distance between them.
2) This law explains phenomena like the orbit of planets around the sun and the moon around Earth. It also explains why objects fall with an acceleration of 9.8 m/s^2 on Earth.
3) The weight of an object, which is the gravitational force exerted by Earth, differs on other celestial bodies due to differences in their masses and radii. Calculations show an object's weight on
Here are the key steps to calculate the mass of Earth (M) from the given data:
1) Acceleration due to gravity on Earth's surface (g) = 9.81 m/s^2
2) Universal gravitational constant (G) = 6.67x10^-11 Nm^2/kg^2
3) Radius of Earth (R) = 6.37x10^6 m
4) Using the formula for acceleration due to gravity:
g = GM/R^2
5) Rearranging the terms:
M = gR^2/G
6) Substituting the values:
M = (9.81 m/s^2)(
Work is done when a force causes an object to be displaced. Work (W) is equal to force (F) multiplied by displacement (s). Work units are joules. Potential energy is stored energy due to an object's position or state. Kinetic energy is the energy of motion and depends on an object's mass and velocity. Power is the rate at which work is done or energy is converted and is measured in watts. Conservation of energy states that energy cannot be created or destroyed, only changed from one form to another.
Karen Adelan presented on the topic of classical mechanics and energy. Some key points:
- Energy is a conserved quantity that can change forms but is never created or destroyed. It is useful for describing motion when Newton's laws are difficult to apply.
- Kinetic energy is the energy of motion and depends on an object's mass and speed. The work-kinetic energy theorem states that the net work done on an object equals the change in its kinetic energy.
- Potential energy is the energy an object possesses due to its position or state. The work done by a constant force equals the product of force, displacement, and the cosine of the angle between them.
posted by Shifat Sanchez..</br>
its about relativity</BR.about sir albert Einstein. quotes about relativity...michelsone and morleys law about relativity....general theory of relativity ..Einstein laws about relativity...Einstein description of laws about theory of special relativity ....first postulates of special law,,sceond postulates of special laws of relativity.........Galilian transformation of relativity....................Lorentz transformation.......... Lorentz transformation about the laws of relativity........Length contractiion .....Time dilation........Mass expansion........E= MC^2 ( theory & provens ))......The life cycle of stars.......Black holes ( slides).............Formation And Properties of blackholes ................Concluation .........Thankyou slide ...............ANY QUESATION ?????????................thank YOU SO MUCH :P :P :P
* Mass of earth (M) = 5.98 x 1024 kg
* Radius of earth (R) = 6378100 m
* Gravitational constant (G) = 6.6726 x 10-11 N-m2/kg2
* Escape velocity (v) = √(2GM/R)
= √(2 x 6.6726 x 10-11 x 5.98 x 1024 / 6378100)
= √(2 x 3.986 x 1014 / 6378100)
= √(2 x 6.273 x 107)
= √1.2546 x 108
= 11.186 km/s
Therefore, the escape
this is class 12 Maharashtra board physics subject content. this is complete content with notes with easily explaination.
for buying or neet attractive ppt in any subject contact me 8879919898. go to my site akchem.tk
blog akchem.blogspot.com
The document discusses concepts related to mechanical energy, including work, kinetic energy, potential energy, and power. It defines energy as the capacity to do work and describes several forms of energy. Work is defined as the dot product of force and displacement. Kinetic energy is defined as 1/2mv^2 and depends on an object's motion. Potential energy exists in gravitational and elastic forms and depends on an object's position or state. The conservation of mechanical energy and work-energy theorem are explained. Power is defined as the rate of energy transfer.
The document discusses collisions and the law of conservation of momentum. It provides examples of how to use a momentum table and algebra to solve for unknown velocities in collision problems involving isolated systems where momentum is conserved. Specifically, it works through examples of a person catching a medicine ball on ice and of two people colliding on an ice rink to determine their combined velocity after collision.
Free fall is the downward motion of objects under the influence of gravity alone. All objects in free fall accelerate at the same rate of 9.8 m/s2 regardless of mass. Experiments show that free-falling objects do not encounter air resistance and accelerate constantly at 9.8 m/s2. Applications of free fall include skydiving and parachuting.
Parallax is the apparent change in position of an object when viewed from different positions. It can be used to measure distances to celestial objects. Stellar parallax involves measuring the difference in the position of a nearby star observed from opposite sides of Earth's orbit around the Sun. This allows astronomers to determine the star's distance using trigonometry. In 1989, the Hipparcos satellite improved parallax measurements for over 100,000 nearby stars. The Gaia satellite, launched in 2013, can measure parallax angles to greater accuracy, mapping stars up to tens of thousands of light years away.
The document discusses several topics related to heat and temperature, including:
1. It defines temperature as a measure of the average kinetic energy of atoms and molecules in a gas or substance, with higher temperatures corresponding to faster molecular motion.
2. It describes different devices that can be used to measure temperature, such as mercury thermometers, gas thermometers, pyrometers, and electrical resistance thermometers.
3. It explains concepts such as heat capacity, specific heat capacity, calorimetry, latent heat, phase changes, conduction, convection, radiation, and Newton's Law of Cooling.
Electric Charge and Electric Field LectureFroyd Wess
More: http://www.pinoybix.org
Lesson Objectives:
Static Electricity; Electric Charge and Its Conservation
Electric Charge in the Atom
Insulators and Conductors
Induced Charge; the Electroscope
Coulomb’s Law
Solving Problems Involving Coulomb’s Law and Vectors
The Electric Field
Field Lines
Electric Fields and Conductors
Gauss’s Law
Electric Forces in Molecular Biology: DNA Structure and Replication
Photocopy Machines and Computer Printers Use Electrostatics
Physics Project On Physical World, Units and MeasurementSamiran Ghosh
This PowerPoint is Physical World, Units and Measurement. This is basically the first chapter of 11th class/grade. This power point explains the basic or fundamental physics with some information about SI units and fundamental forces.
This document introduces the topic of electrostatics and electric charges and fields. Some key points include:
- Electrostatics deals with static electric charges and the forces, fields, and potentials arising from them. Charges can be positive or negative.
- The electric field is a vector quantity that describes the force exerted on a charge in a given point in space. It is calculated using Coulomb's law and the superposition principle.
- Electric field lines are imaginary lines used to depict electric fields graphically. They originate on positive charges and terminate on negative charges.
- Gauss's law relates the electric flux through a closed surface to the net charge enclosed by the surface. It can be used to calculate electric
The document provides information about current, electromotive force, potential difference, and resistance. It defines key terms, provides equations, and examples of calculations. It describes:
- Current is the flow of charge measured in amperes. It is carried by the flow of electrons in a conductor.
- Electromotive force is the work done per unit charge to drive charge around a complete circuit. It is measured in volts.
- Potential difference is the work done per unit charge to move charge through a circuit component. It is also measured in volts.
- Resistance is the opposition to current flow. It is calculated as potential difference divided by current and measured in ohms.
The center of mass of an object is the single point where the entire mass of the object is considered to be concentrated and acts as if the whole mass were located; it is defined mathematically as the weighted average of every discrete point making up the object. The document discusses center of mass for different geometric objects like cylinders, spheres, and distributed point masses, and explains that finding the center of mass allows predicting the object's motion as if all its mass were concentrated at that point.
Digital Library of GLT Saraswati Bal Mandir. Gravitation is a natural phenomenon by which all physical bodies attract each other. It is most commonly experienced as the agent that gives weight to objects with mass and causes them to fall to the ground when dropped.
Gravitation has been the most common phenomenon in our lives but somewhere down the line we don't know musch about it. So here is a presentation whic will help you out to know what it is !! I'll be makin it available for download once i submit it in school :P :P ! Coz last one of the brats showed the same presentation that i uploade and unfortunatele his roll number fell before mine ! I was damned..:D :D :P
This document provides an overview of Mumbai University, the application of computers in education, information and communication technology (ICT) in education, optical mark recognition (OMR), and the history and mechanism of OMR. Mumbai University was introduced in 1857 and has two campuses located in Mumbai, India. It offers various degrees and was ranked 41st in the world and 5th in India in 2013. ICT and computers play a vital role in the education sector by providing quick access to information, connecting dispersed regions, and catering to individual differences. OMR is a scanning technology used to read and evaluate questionnaires, surveys, and tests with pre-printed answer fields. It has advantages such as simplicity and high speed but cannot recognize hand
This document discusses Kepler's laws of planetary motion and Newton's universal law of gravitation. It also describes how gravitational acceleration varies with altitude, depth, and latitude on Earth. Some key points covered include:
1) Kepler analyzed Tycho Brahe's planetary data and discovered three laws, including that planets orbit in ellipses with the Sun at one focus.
2) Newton's law states that the gravitational force between two objects is directly proportional to their masses and inversely proportional to the square of the distance between them.
3) Gravitational acceleration decreases with altitude and depth from Earth's surface, and is lowest at the equator due to centrifugal effects.
This document contains 80 questions related to digital signal and image processing. The questions cover topics such as image transforms, filters, noise, compression, segmentation, and more. Justification is required for some questions, while others involve calculations, derivations or explanations of key concepts. The questions vary in difficulty and mark allocation from 5 to 10 marks. They also specify the exam or year in which the question appeared previously.
The document discusses constructor overloading in Java using a Box class. It defines multiple constructors for the Box class that take different parameters, allowing objects to be initialized in different ways. It then defines a BoxMass subclass that inherits from Box and adds a mass property. The main method demonstrates creating BoxMass objects with different constructors and printing their volume and mass. It also discusses using a superclass reference variable to reference a subclass object, and the limitations this introduces. Finally, it covers using the super keyword in subclass constructors to call parent constructors and access hidden superclass members.
This document discusses concepts related to gravitation and satellites. It begins with an overview of Newton's law of gravitation, including definitions of the gravitational constant G. It then discusses how G relates to the acceleration due to gravity g. Several concepts pertaining to satellites are covered, including the critical velocity required for satellites to orbit Earth, their orbital periods, and factors that affect these values. The document also examines weightlessness in satellites and the escape velocity required for a satellite to break free of Earth's gravitational pull.
Social media is online communication channels used for sharing information among friends and communities. Popular social media sites include Facebook, Twitter, YouTube, and LinkedIn. Flipkart, an Indian e-commerce company, uses various social media platforms for purposes like marketing, promotions, customer engagement, and hiring. LinkedIn is used for talent acquisition and networking, while Twitter, YouTube and Facebook are used to connect with customers, advertise products, and build the Flipkart brand. Pinterest allows Flipkart to visually market products and leverage social sharing.
The document provides an overview of the Java Database Connectivity (JDBC) API. It describes key interfaces like Connection, Statement, and PreparedStatement that are used to connect to a database and execute SQL statements. It also covers ResultSet for accessing query results, and the use of transactions and savepoints for maintaining data integrity. Classes like DriverManager help establish the initial connection to access databases using JDBC.
1. The document discusses logarithmic tables and how they can be used to perform calculations without a calculator.
2. Logarithmic tables allow users to look up the logarithm of a number and then use logarithmic properties to simplify complex calculations into addition or subtraction.
3. Examples are provided to demonstrate how to use logarithmic tables to find logarithms, multiply and divide numbers, take square roots, and perform other calculations.
The document discusses communication protocols and the OSI model. It defines what a communication protocol is and explains the reasons for using layered protocols. The key advantages of layering are also outlined. The seven layers of the OSI model are described along with the functions of the physical and data link layers. The differences between network layer delivery and transport layer delivery are explained. Finally, some common networking terms like logical address, physical address, and port address are defined.
This document contains solutions to 5 questions about orbital mechanics. Question 1 calculates the centripetal and centrifugal accelerations, velocity, and orbital period of a satellite in a 1,400 km circular orbit. Question 2 does similar calculations for a 322 km circular orbit, finding the orbital angular velocity, period, and velocity. Question 3 calculates Doppler shifts for signals from this satellite received by observers in space and on the Earth's surface. Question 4 states Kepler's laws of planetary motion and uses the third law to find the orbital period of a satellite in an elliptical orbit with a 39,152 km apogee and 500 km perigee.
1) A flowchart is a graphical representation of an algorithm or process that uses standard symbols to indicate the flow of logic and sequence of steps.
2) Flowcharts are useful for documenting and understanding complex logic in a language-independent way. They can represent sequential statements, branching, looping, and other control structures.
3) Guidelines for drawing flowcharts include using standard symbols, maintaining logical sequence from top to bottom, and ensuring only one line enters decision points while multiple lines can leave.
This document discusses circular motion and provides examples and explanations of key concepts related to circular motion, including:
1) Circular motion is defined as motion along a complete or partial circle. Centripetal force is required to produce the acceleration needed for circular motion.
2) Examples of centripetal force include tension in a string for a body whirled in a circle, friction for a car rounding a turn, and gravitational attraction for objects like moons orbiting planets.
3) Centripetal acceleration always points toward the center of the circular path and has a magnitude of v^2/r, where v is the object's speed and r is the radius of the path. Radial acceleration equals the
This document discusses different techniques for reading files in Python. It begins by explaining what files are and the different types, with a focus on text files. It then demonstrates opening a file and reading the entire contents in one string. Next, it shows how to read each line of a file as a separate string using readlines(). Finally, it provides an example of printing the lines of a file in reverse order to illustrate reading files in different ways. The key techniques covered are reading the entire file, reading a specified number of characters, reading each line as a separate string, and iterating through the lines in reverse order.
2.1 form 3 simple kinetic molecular model of matterchris lembalemba
This document describes the kinetic molecular model of matter. It explains that matter exists in three states - solid, liquid, and gas - depending on how tightly or loosely bound the particles are and how much they move. Solids have a fixed shape and volume as particles vibrate in place. Liquids have no fixed shape but a fixed volume as particles move past each other. Gases have no fixed shape or volume as particles move freely in all directions at high speeds with little attraction. Higher temperatures means particles have more kinetic energy and evaporation occurs when the most energetic particles overcome attractive forces and escape as a gas.
There are two main sources of energy: conventional and non-conventional. Conventional sources include fossil fuels like coal, petroleum and natural gas. However, burning fossil fuels causes air and water pollution and global warming. Non-conventional renewable sources include solar, wind, hydropower, biomass and ocean energies. These are better for the environment as they don't cause pollution, but have other disadvantages like high initial costs, need for large land areas, and variability in availability. Overall sources of energy must be evaluated based on the ease and costs of extraction as well as their environmental impacts.
Cm 3 centripetal force & acceleration (shared)LThistlewood
This document provides an overview of a physics lesson on centripetal force and acceleration. It introduces the key equations for centripetal acceleration (a = v2/r) and centripetal force (F = mv2/r). The learning objectives are to use these two equations and solve basic problems using them. The document then derives the equations step-by-step, showing the relationship between centripetal acceleration and the change in velocity of an object moving in circular motion.
This document discusses uniform circular motion. It defines uniform circular motion as motion along a circular path with constant speed. It describes key concepts like centripetal acceleration, which is directed radially inward, and centripetal force, which provides the inward force needed for uniform circular motion. Several example problems are worked through applying concepts like centripetal force and centripetal acceleration to situations involving objects moving in circular paths.
This document contains lecture notes on various topics related to gravitation and orbital mechanics:
1. It defines Newton's law of gravitation and the gravitational constant G.
2. It discusses the difference between G and g, the acceleration due to gravity, and derives the relation between the two.
3. It then covers concepts like the critical velocity, time period, binding energy, and escape velocity required for a satellite to orbit or escape the gravitational pull of Earth.
4. Additional topics include weightlessness in satellites, variation of g with altitude and depth, and the definition of latitude.
This document provides an overview of key concepts in gravitation including: the definition of gravitation; Newton's law of universal gravitation; acceleration due to gravity and how it varies with height and depth; escape velocity; orbital velocity; gravitational potential; time period of satellites; Kepler's laws of planetary motion; and types of satellites. Key points covered include how gravity decreases with height but increases with depth below the Earth's surface, and definitions of geostationary, polar, and binding energy as they relate to satellites orbiting the Earth.
In physics, gravity (from Latin gravitas 'weight'[1]) is a fundamental interaction which causes mutual attraction between all things that have mass. Gravity is, by far, the weakest of the four fundamental interactions, approximately 1038 times weaker than the strong interaction, 1036 times weaker than the electromagnetic force and 1029 times weaker than the weak interaction. As a result, it has no significant influence at the level of subatomic particles.[2] However, gravity is the most significant interaction between objects at the macroscopic scale, and it determines the motion of planets, stars, galaxies, and even light.
On Earth, gravity gives weight to physical objects, and the Moon's gravity is responsible for sublunar tides in the oceans (the corresponding antipodal tide is caused by the inertia of the Earth and Moon orbiting one another). Gravity also has many important biological functions, helping to guide the growth of plants through the process of gravitropism and influencing the circulation of fluids in multicellular organisms.
The gravitational attraction between the original gaseous matter in the universe caused it to coalesce and form stars which eventually condensed into galaxies, so gravity is responsible for many of the large-scale structures in the universe. Gravity has an infinite range, although its effects become weaker as objects get farther away.
Gravity is most accurately described by the general theory of relativity (proposed by Albert Einstein in 1915), which describes gravity not as a force, but as the curvature of spacetime, caused by the uneven distribution of mass, and causing masses to move along geodesic lines. The most extreme example of this curvature of spacetime is a black hole, from which nothing—not even light—can escape once past the black hole's event horizon.[3] However, for most applications, gravity is well approximated by Newton's law of universal gravitation, which describes gravity as a force causing any two bodies to be attracted toward each other, with magnitude proportional to the product of their masses and inversely proportional to the square of the distance between them.
Current models of particle physics imply that the earliest instance of gravity in the universe, possibly in the form of quantum gravity, supergravity or a gravitational singularity, along with ordinary space and time, developed during the Planck epoch (up to 10−43 seconds after the birth of the universe), possibly from a primeval state, such as a false vacuum, quantum vacuum or virtual particle, in a currently unknown manner.[4] Scientists are currently working to develop a theory of gravity consistent with quantum mechanics, a quantum gravity theory,[5] which would allow gravity to be united in a common mathematical framework (a theory of everything) with the other three fundamental interactions of physics.
Newton's theory of universal gravitation proposes that every object in the universe attracts every other object with a force proportional to the product of their masses and inversely proportional to the square of the distance between them. Newton realized that the moon and falling apples are attracted to Earth by the same force of gravity. He determined gravitational forces exist between all objects and derived the inverse-square law formula to calculate these forces. Examples of applying Newton's theory include calculating the masses of Earth and Sun from their gravitational interactions, and determining satellite speeds and orbital distances using formulas balancing gravitational and centrifugal forces.
Gravitation is a force that attracts two masses towards each other. Newton's Law of Universal Gravitation states that the gravitational force between two objects is directly proportional to the product of their masses and inversely proportional to the square of the distance between them. Albert Einstein later developed the theory of gravitation further in his theories of relativity. On Earth, the acceleration due to gravity is approximately 9.8 m/s2, causing objects to fall towards the ground when dropped.
1) There are four main types of forces - gravitational, electromagnetic, nuclear, and centripetal. Gravitational force acts between any two masses and depends on their masses and the distance between them.
2) Kepler's laws of planetary motion describe the motion of planets in the solar system. Newton's universal law of gravitation states that there is a gravitational attraction between any two masses that is directly proportional to the product of their masses and inversely proportional to the square of the distance between them.
3) Gravitational acceleration (g) is the acceleration on an object due to gravity. On Earth, g is approximately 9.8 m/s2. The value of g depends on factors like the
Gravitation, free fall, variation in 'g' and keplers law lecture wiseRohan Jain
This document contains lecture notes on gravitational force and Newton's law of universal gravitation. It discusses key topics including:
- Gravitational force is a fundamental force that attracts all objects with mass. Newton's law of gravitation describes the force as directly proportional to the product of the masses and inversely proportional to the square of the distance between them.
- Kepler's laws of planetary motion describe how planets move in elliptical orbits with the sun at one focus. Kepler's first law states orbits are ellipses, the second that planets sweep out equal areas in equal times, and the third relates orbital periods to orbital radii.
- The value of the gravitational acceleration g varies depending on location, altitude,
- Newton proposed his law of universal gravitation, which states that every particle in the universe attracts every other particle with a force directly proportional to the product of their masses and inversely proportional to the square of the distance between them.
- The gravitational field strength is defined as the gravitational force exerted per unit mass. Near the surface of planets like Earth, the gravitational field strength equals the acceleration due to gravity.
- Kepler's laws describe the motion of planets in the solar system, including that planets move in elliptical orbits with the sun at one focus, and the time to sweep out equal areas is equal.
This document discusses satellite communication and related concepts. It covers topics like satellite orbits and trajectories, including orbital parameters, types of orbits, and factors that affect a satellite's performance. It also discusses the basic principles governing satellite motion, Kepler's laws of planetary motion, and concepts like injection velocity and orbital trajectories. The goal is to help students understand the technologies associated with satellite communication systems.
- The Energy is found alone before any Matter Creation
- A general Energy is found before the solar planets creation (I called this Energy "The Mother Energy")
- This mother Energy creates the solar planets matters (Mass) and orbital distances (Space)
- The Mother Energy forces the solar planet to move following her motion, So the planet follows the Energy Motion trajectory (with different rate of time)
That answers the question
- Why Earth circumference =40080 km?
1. The document discusses concepts related to gravitation including Newton's universal law of gravitation, Kepler's laws of planetary motion, acceleration due to gravity, mass, weight, thrust, pressure, and equations of vertical motion.
2. Key figures discussed include Johannes Kepler, Isaac Newton, and Archimedes. Newton developed the universal law of gravitation and Kepler described three empirical laws of planetary motion.
3. The universal law of gravitation states that the gravitational force between two objects is directly proportional to the product of their masses and inversely proportional to the square of the distance between them.
Gravity is a mysterious force that attracts all objects with mass, even when far apart. Newton discovered that all objects accelerate towards Earth at 9.81 m/s2, and the moon accelerates towards Earth at 2.72 m/s2. Gravity is weak but exists between all objects, causing dust in space to come together to form stars and planets.
Maths and Astronomy Why Maths Comenius projectGosia Garkowska
This document discusses various topics related to math and astronomy. It begins by introducing distance units used in space like astronomical units (AU), light years, parsecs and larger multiples. It then discusses how to calculate acceleration due to gravity on different planets using Newton's law of universal gravitation. Next, it examines weight on other planets and how gravity differs based on planetary characteristics. The document concludes by calculating the orbital speeds of planets around the sun.
1. The document discusses key concepts of gravitation including Newton's universal law of gravitation, Kepler's laws of planetary motion, gravitational force, acceleration due to gravity, escape velocity, and free fall.
2. It explains that gravitational force is responsible for holding the atmosphere above the earth and for the motion of objects.
3. Newton's universal law of gravitation states that the gravitational force between two objects is directly proportional to the product of their masses and inversely proportional to the square of the distance between them.
This document discusses Sir Isaac Newton and Johannes Kepler's contributions to the understanding of gravitation. It covers Newton's universal law of gravitation, Kepler's laws of planetary motion, gravitational force, acceleration due to gravity, equations of vertical motion, mass, weight, thrust, pressure, Archimedes' principle, and density. Key points include Newton's inverse square law of gravitation, Kepler's three laws of planetary motion, how gravitational force causes objects to accelerate at 9.8 m/s2 on Earth, and how pressure depends on both force and contact area.
1) Newton proposed that all objects with mass 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.
2) An object in free fall experiences a sensation of weightlessness because both it and the elevator/spacecraft it is in are accelerating downward at the same rate due to gravity, so there is no relative acceleration between them.
3) A satellite in orbit around a planet is weightless because the centripetal acceleration needed to maintain its orbit exactly counteracts the acceleration due to gravity, resulting in no net acceleration felt by objects in the spacecraft.
- The document discusses Newton's formulation of the universal law of gravitation and its importance.
- Newton realized that the same force responsible for objects falling on Earth was also responsible for the motion of planets and the moon. This force is gravitational force.
- The universal law of gravitation states that every object in the universe attracts every other object with a force proportional to the product of their masses and inversely proportional to the square of the distance between them.
- The law successfully explained phenomena like the motion of planets, moons, and tides, and established that gravitational force existed between all bodies in the universe.
- The document discusses Newton's law of gravitation and Kepler's laws of planetary motion.
- Newton's law of gravitation states that the gravitational force between two objects is directly proportional to the product of their masses and inversely proportional to the square of the distance between them.
- Kepler's laws describe the motion of planets in the solar system, including that planets move in elliptical orbits with the sun at one focus, their radius vectors sweep out equal areas in equal times, and the squares of their orbital periods are proportional to the cubes of their semi-major axes.
The Elphinstonian 1988-College Building Centenary Number (2).pdfMukesh Tekwani
This is the 1988 issue of The Elphinstonian, the annual magazine of Elphinstone College, Mumbai. This is the special issue to commemorate the Century of the Elphinstone College Building in Mumbai.
ISCE-Class 12-Question Bank - Electrostatics - PhysicsMukesh Tekwani
This is a 14 page question bank on the chapters of Electrostatics. This is based on the syllabus of most Board exams such as CBSE, ISCE and state boards.
Extremely important topic for Digital electronics, digital circuits, computer architecture and computer science.
Full video is available on Youtube: https://youtu.be/oyOaXqx06pY
This video explains the method of converting a decimal number to a binary number. Many solved examples are given here and also two exercises which you can attempt on your own and then check the answers.
I have also discussed the concept of LSB (least significant bit) and MSB (most significant bit), and also least significant digit (LSD) and most significant digit (MSD).
This topic is important for following courses: class 11 and 12 computer science of all state boards, class 11 and 12 physics, BSc Computer science, BSc IT, MCA (Masters degree in Computer Applications), BTech, BE (First Year), and many competitive examinations.
Free Lectures on YouTube for IGCSE Physics for the syllabus effective 2020-21. These lectures cover the syllabus of IGCSE and a major part of GCSE syllabus also.
1. The Hidden Meaning of Words in Science Question Papers
2. Scientific Notation or Powers of Ten Notation
3. Units and Base Quantities
4. What is Physics?
Refraction and dispersion of light through a prismMukesh Tekwani
This document contains 20 important theory questions about refraction and dispersion of light through a prism. Some key topics covered are:
1) The angle of deviation of light passing through a prism depends on factors like the refracting angle of the prism and the angle of incidence of light.
2) When white light passes through a prism, it disperses into its constituent colors due to the refractive index of the material being different for different wavelengths of light.
3) In the position of minimum deviation, the angles of incidence and refraction of a monochromatic light ray passing through a prism are related to the refracting angle of the prism.
This document contains important theory questions about refraction of light at a plane surface and total internal reflection. It includes 24 multiple choice and derivation questions covering topics such as Snell's law, refractive index, critical angle, total internal reflection, mirages, reflecting prisms, reversing prisms, erecting prisms, optical fibers, and their applications. The document was prepared by Mukesh N Tekwani and provides a comprehensive review of key concepts and formulas relating to the refraction and total internal reflection of light.
This document contains 10 important theory questions about spherical mirrors. It defines key terms used to describe spherical mirrors such as pole, center of curvature, radius of curvature, principal axis, aperture, principal focus, focal length and focal plane. It also derives several important relationships for spherical mirrors, including that the focal length of a concave or convex mirror of small aperture is half the radius of curvature, and the mirror formula relating the focal length to the object and image distances. Finally, it derives the magnification formula for concave mirrors and asks which type of spherical mirror is preferable for observing traffic from a car.
Atom, origin of spectra Bohr's theory of hydrogen atomMukesh Tekwani
This document contains 15 important theory questions about Rutherford's alpha particle scattering experiment, Rutherford's model of the atom, its limitations, Bohr's model of the hydrogen atom, Bohr's postulates, expressions for the stationary and kinetic energy levels of an electron in the hydrogen atom, the energy level diagram for hydrogen showing different emission series, and definitions of terms like Rydberg constant, excitation potential, and ionization potential. The questions are related to key experiments and models in the development of atomic structure and spectra.
Refraction of light at spherical surfaces of lensesMukesh Tekwani
This document contains 15 important theory questions about refraction of light at spherical surfaces and lenses. It includes questions about sign convention in optics, the optical center of a lens, focal length of concave and convex lenses, lens maker's formula, derivation of expressions for refraction at single spherical surfaces and thin lens combinations, linear magnification by a lens, location of a virtual image formed by a convex lens based on focal length, dependence of focal length on wavelength, definition and unit of power of a lens, definition of 1 dioptre, formula for combined power of two lenses in contact, and laws governing image formation by lenses. The questions cover key concepts like derivation, definition, diagrams, formulas, and image formation.
This document outlines the unit-wise weightage for the February 2020 ISCE Class 12 Physics board exam. Unit 3 on Magnetic Effects of Current and Magnetism has the highest weightage at 16. Other highly weighted units include Electromagnetic Induction and Alternating Currents at 14, and Optics at 12. The lowest weighted units are Communication Systems at 2 and Electronic Devices at 8.
What is Cyber Law? Why is cyber security law needed? International cyber law. What is copyright? What are security, controls, privacy, piracy and ethics? Code of ethics for computer professionals. What is cyber insurance?
The document discusses the disadvantages of HTML and the advantages of using XML instead. It notes that HTML lacks structure, syntax checking, and is not suitable for data interchange or describing semantics. XML was designed to store, describe, and transport data, unlike HTML which was designed for display. XML simplifies data sharing and transport between applications since it separates data from presentation and uses plain text. It also allows for international character support and makes data more available and reusable.
This presentation discusses various social media platforms and provides information on social media, social media analytics, and social media marketing. It defines social media as online communication channels used for sharing content and collaboration. It explains that social media analytics involves gathering and analyzing data from social media sites to make business decisions. Social media marketing aims to create shareable content to expose brands and increase reach. The presentation then outlines popular social media platforms like Facebook, Twitter, LinkedIn, Wikipedia and Pinterest, describing their basic uses and features. It concludes with discussing precautions to take when using these social media sites.
A review of the growth of the Israel Genealogy Research Association Database Collection for the last 12 months. Our collection is now passed the 3 million mark and still growing. See which archives have contributed the most. See the different types of records we have, and which years have had records added. You can also see what we have for the future.
Physiology and chemistry of skin and pigmentation, hairs, scalp, lips and nail, Cleansing cream, Lotions, Face powders, Face packs, Lipsticks, Bath products, soaps and baby product,
Preparation and standardization of the following : Tonic, Bleaches, Dentifrices and Mouth washes & Tooth Pastes, Cosmetics for Nails.
Exploiting Artificial Intelligence for Empowering Researchers and Faculty, In...Dr. Vinod Kumar Kanvaria
Exploiting Artificial Intelligence for Empowering Researchers and Faculty,
International FDP on Fundamentals of Research in Social Sciences
at Integral University, Lucknow, 06.06.2024
By Dr. Vinod Kumar Kanvaria
How to Build a Module in Odoo 17 Using the Scaffold MethodCeline George
Odoo provides an option for creating a module by using a single line command. By using this command the user can make a whole structure of a module. It is very easy for a beginner to make a module. There is no need to make each file manually. This slide will show how to create a module using the scaffold method.
বাংলাদেশের অর্থনৈতিক সমীক্ষা ২০২৪ [Bangladesh Economic Review 2024 Bangla.pdf] কম্পিউটার , ট্যাব ও স্মার্ট ফোন ভার্সন সহ সম্পূর্ণ বাংলা ই-বুক বা pdf বই " সুচিপত্র ...বুকমার্ক মেনু 🔖 ও হাইপার লিংক মেনু 📝👆 যুক্ত ..
আমাদের সবার জন্য খুব খুব গুরুত্বপূর্ণ একটি বই ..বিসিএস, ব্যাংক, ইউনিভার্সিটি ভর্তি ও যে কোন প্রতিযোগিতা মূলক পরীক্ষার জন্য এর খুব ইম্পরট্যান্ট একটি বিষয় ...তাছাড়া বাংলাদেশের সাম্প্রতিক যে কোন ডাটা বা তথ্য এই বইতে পাবেন ...
তাই একজন নাগরিক হিসাবে এই তথ্য গুলো আপনার জানা প্রয়োজন ...।
বিসিএস ও ব্যাংক এর লিখিত পরীক্ষা ...+এছাড়া মাধ্যমিক ও উচ্চমাধ্যমিকের স্টুডেন্টদের জন্য অনেক কাজে আসবে ...
Strategies for Effective Upskilling is a presentation by Chinwendu Peace in a Your Skill Boost Masterclass organisation by the Excellence Foundation for South Sudan on 08th and 09th June 2024 from 1 PM to 3 PM on each day.
How to Fix the Import Error in the Odoo 17Celine George
An import error occurs when a program fails to import a module or library, disrupting its execution. In languages like Python, this issue arises when the specified module cannot be found or accessed, hindering the program's functionality. Resolving import errors is crucial for maintaining smooth software operation and uninterrupted development processes.
How to Manage Your Lost Opportunities in Odoo 17 CRMCeline George
Odoo 17 CRM allows us to track why we lose sales opportunities with "Lost Reasons." This helps analyze our sales process and identify areas for improvement. Here's how to configure lost reasons in Odoo 17 CRM
This presentation was provided by Steph Pollock of The American Psychological Association’s Journals Program, and Damita Snow, of The American Society of Civil Engineers (ASCE), for the initial session of NISO's 2024 Training Series "DEIA in the Scholarly Landscape." Session One: 'Setting Expectations: a DEIA Primer,' was held June 6, 2024.
Introduction to AI for Nonprofits with Tapp NetworkTechSoup
Dive into the world of AI! Experts Jon Hill and Tareq Monaur will guide you through AI's role in enhancing nonprofit websites and basic marketing strategies, making it easy to understand and apply.
How to Add Chatter in the odoo 17 ERP ModuleCeline George
In Odoo, the chatter is like a chat tool that helps you work together on records. You can leave notes and track things, making it easier to talk with your team and partners. Inside chatter, all communication history, activity, and changes will be displayed.
3. Newton’s Law of Gravitation
Every particle of matter attracts every other
particle with a force which is directly
proportional to the product of the masses
and inversely proportional to the square of
the distance between them.
Prof. Mukesh N Tekwani
3
4. Newton’s Law of Gravitation
G is called the Universal Gravitational
Constant
G = 6.67 x 10-11 N m2/kg2
G is constant throughout the Universe and G
does not depend on the medium Mukesh N Tekwani the
between
Prof.
4
5. Difference between G and g
G
G is the Universal
Gravitational Constant
G = 6.67 x 10-11 N m2/kg2
Constant throughout the
Universe
g
g is acceleration due to
gravity
Approx value g = 9.8 m /
s2.
Value of g varies from one
place to another on the
Earth.
Changes every place on a
planet. E.g., on the Moon,
the value of g is 1/6th of
that on the Earth’s
surface.
Prof. Mukesh N Tekwani
5
6. Relation between G and g
Let M = mass of the Earth
m = mass of an object on the surface
of the Earth
g = acceleration due to gravity on the
Earth’s surface
R = radius of the Earth
Prof. Mukesh N Tekwani
6
8. Relation between G and g
m
M
Weight of the object is the
gravitational force acting on
it.
………………………….(1)
Prof. Mukesh N Tekwani
8
9. Relation between G and g
At height h from the surface of the
Earth’s surface, acceleration due to
gravity is gh
m
h
M
At height h,
Weight of object = gravitational force
………………………….(2)
Prof. Mukesh N Tekwani
9
10. Relation between G and g
Dividing (2) by (1) we get,
m
h
M
Thus, g is independent of the mass of
the object.
Prof. Mukesh N Tekwani
10
11. Projection of a Satellite
Why is it necessary to have at least a two stage
rocket to launch a satellite?
A rocket with at least two stages is required to
launch a satellite because
The first stage is used to carry the satellite up
to the desired height.
In the second stage, rocket is turned
horizontally (through 90 degrees) and the
satellite is fired with the proper horizontal
velocity to perform circular motion around the
earth.
Prof. Mukesh N Tekwani
12
12. Critical Velocity of a Satellite
The horizontal velocity
with which a satellite
should be projected from
a point above the earth's
surface, so that it orbits
in a circular path around
the earth is called the
orbital velocity or critical
velocity (Vc) of the
satellite.
Prof. Mukesh N Tekwani
13
13. Kepler’s Laws of Motion
Born:
December 27, 1571
Died:
November 15, 1630
German
Mathematician,
Astronomer
Astrologer.
Prof. Mukesh N Tekwani
14
14. Kepler’s First Law – Law of Orbit
Every planet revolves in an elliptical
orbit around the Sun, with the Sun
situated at one focus of the ellipse.
Prof. Mukesh N Tekwani
15
15. Kepler’s Second Law
or Law of Equal Areas
The radius vector drawn from the
Sun to any planet sweeps out equal
areas in equal intervals of time. This
law is called the law of areas.
The areal velocity of the radius vector
is constant.
Prof. Mukesh N Tekwani
16
18. Kepler’s Third Law - Laws of
Period
The square of period of revolution of
the planet around the Sun is directly
proportional to the cube of the semimajor axis of the elliptical orbit.
T2 α r3
According to this law, when the planet is
closest to the Sun, its speed is maximum
and when it is farthest from the Sun, its
speed is minimum.
Prof. Mukesh N Tekwani
19
19. Critical Velocity of a Satellite
Let
vc
h
R
M
r
M = mass of the
Earth
R = radius of Earth
m = mass of satellite
h = height of the
satellite above
Earth’s
r = R + h, where r is
the distance of the
satellite from the
center of the Earth
Vc = critical velocity
Prof. Mukesh N Tekwani
of the satellite
20
20. Critical Velocity of a Satellite
The centripetal force necessary for the circular
motion of the satellite around the Earth is provided
by the gravitational force of attraction between the
Earth and the satellite.
Centripetal force = gravitational force
Prof. Mukesh N Tekwani
21
21. Critical Velocity of a Satellite
……………………………………………….(1)
Factors on which Critical Velocity of a satellite
depends:
1. Mass of the planet
2. Radius of the planet
3. Height of the satellite
Critical velocity is not dependent on the mass of the
satellite as m does not appear in the above
equation
Prof. Mukesh N Tekwani
22
22. Critical Velocity of a Satellite
But we know that
Substituting this value in eqn (1), we get,
…………………………………..(2)
Prof. Mukesh N Tekwani
23
23. Critical Velocity of a Satellite
Assignment 1:
Modify eqn (2) to find the critical velocity of a
satellite orbiting very close to the surface of the
Earth (h << R)
Assignment 2:
How does the critical velocity (or orbital velocity) of
a satellite vary with an increase in the height of the
satellite above the Earth’s surface?
Prof. Mukesh N Tekwani
24
24. Time Period of a Satellite
The time taken by a satellite to
complete one revolution around the
earth is called its periodic time or time
period.
Prof. Mukesh N Tekwani
25
25. Time Period of a Satellite
Let
vc
h
R
M
r
M = mass of the
Earth
R = radius of Earth
m = mass of satellite
h = height of the
satellite above
Earth’s
r = R + h, where r is
the distance of the
satellite from the
center of the Earth
Vc = critical velocity
Prof. Mukesh N Tekwani
of the satellite
26
26. Time Period of a Satellite
Distance covered by the satellite in 1 revolution
= Circumference of the circle
Time taken to cover this distance is the time period
Critical speed Vc =
Vc =
But
Prof. Mukesh N Tekwani
27
27. Time Period of a Satellite
As
Squaring both sides, we get
is a constant,
so we get,
T2 α r3
Thus, the square of the
period of revolution is
directly proportional to
the cube of the radius of
its orbit.
Prof. Mukesh N Tekwani
28
28. Time Period of a Satellite
Factors on which Time Period of a satellite depends:
1. Mass of the planet
2. Radius of the planet, and
3. Height of the satellite from the planet’s surface
Period of the satellite does not depend on the mass
of the satellite.
Assignment:
(1)Obtain an expression for the time period of a
satellite in terms of gh.
(2)For a satellite close to the earth, calculate the
period of revolution in minutes.
Prof. Mukesh N Tekwani
29
29. Binding Energy of a Satellite
Definition:
The minimum amount of energy
required to remove a satellite from the
earth’s gravitational influence is called
as binding energy of the satellite.
A satellite revolving around the Earth
has
Kinetic energy, and
Potential energy
Prof. Mukesh N Tekwani
30
30. What is kinetic energy?
The energy possessed by a body due
to its motion is called its kinetic
energy.
If m = mass of an object, and
v = its velocity
K.E = (1/2) mv2
Prof. Mukesh N Tekwani
31
31. What is potential energy?
The energy possessed by a body due
to its position is called its potential
energy.
If m = mass of an object, and
h = its height above the surface
P.E. = mgh
Quiz: Does a body in motion have
potential energy?
Prof. Mukesh N Tekwani
32
32. Binding Energy of a Satellite
Let
vc
h
R
M
r
M = mass of the
Earth
R = radius of Earth
m = mass of satellite
h = height of the
satellite above
Earth’s
r = R + h, where r is
the distance of the
satellite from the
center of the Earth
Vc = critical velocity
Prof. Mukesh N Tekwani
of the satellite
33
33. Binding Energy of a Satellite
The critical velocity is given by
……………………………………………………...(1
)
Kinetic energy of motion KE =
…..……...(2)
Substituting (1) in (2), we get,
KE =
..………………………………………………..(3
)
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34. Binding Energy of a Satellite
The gravitational potential at a distance r
from the centre of the Earth is given by:
GP =
Potential energy = gravitational potential x
mass of the satellite
Therefore, PE =
..…….………………………..(4
)
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35. Binding Energy of a Satellite
The total energy of the satellite is given by
TE = KE + PE
TE =
TE =
+
..…….…………………………………………..(5)
The negative sign indicates that the satellite
is bound to the Earth due to the gravitational
force of the Earth.
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36. Binding Energy of a Satellite
To free the satellite from the Earth’s
gravitational influence, an amount of energy
equal to its total energy must be supplied.
This is called the binding energy of the
satellite.
Therefore, BE =
Where r = R + h
Assignment: Calculate the BE of a satellite
at rest on the surface of the Earth. N Tekwani
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37. Weightlessness in a Satellite
1. The weight of a body is the gravitational
force exerted on it by the Earth.
2. When a person stands on a floor, he exerts
a force on the floor. The floor in turn exerts
a force (normal reaction) on the person.
3. This normal reaction is equal to the weight
of the person.
4. The person has a feeling of weight due to
this normal reaction.
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38. Weightlessness in a Satellite
5. Consider an astronaut of mass m, in a
satellite that is moving around the Earth in a
circular orbit.
6. There is a centripetal force on the satellite
and the astronaut. Thus, both are attracted
towards the Earth with the same
acceleration, due to the Earth’s gravitational
force.
7. So the astronaut is not able to exert a force
on the floor of the satellite & the satellite in
turn cannot exert normal reaction on the
Prof. Mukesh N Tekwani
astronaut. This causes the “feeling” of
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39. Weightlessness in a Satellite
8. We must remember that the mass of the
astronaut DOES NOT become zero.
9. This condition of weightlessness is also
known (incorrectly) as zero gravity
condition.
10.But, weightlessness does not mean the
absence of gravity.
Prof. Mukesh N Tekwani
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40. Escape Velocity of a Satellite
The minimum
velocity with which
a body should be
projected from the
surface of the
earth so that it
escapes the
gravitational field
of the earth is
called the escape
velocity of the
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41. Escape Velocity of a Satellite
Consider a satellite of mass m,
stationary on the surface of the Earth.
The binding energy of the satellite, on
the surface of the Earth, is given by
BE =
R
To escape from the Earth’s influence,
energy must be provided to the
satellite in the form of kinetic energy.
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42. Escape Velocity of a Satellite
Therefore, KE of satellite = BE
KE =
R
Therefore,
=
R
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43. Numerical Problems
Obtain an equation for the escape
velocity of a body from the surface of
a planet of radius R and mean density
ρ.
What would be the duration of the year if
the distance between the Earth and Sun
gets doubled?
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44. Numerical Problems
Calculate the height of a
communications satellite from the
surface of the Earth. Values of G, M and
R are as given in the text book. (These
values will also be provided in the
question paper)
A body weighs 4.5 kgwt on the surface of
Earth. How much will it weigh on the
surface of a planet whose mass is (1/9)th
that of the Earth’s mass and radius is
half that of the Earth?
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45. Variation of g with Altitude
Weight of the object is the
gravitational force acting on
it.
m
M
………………………….(1)
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46. Variation of g with Altitude
At height h from the surface of the
Earth’s surface, acceleration due to
gravity is gh
m
h
M
At height h,
Weight of object = gravitational force
………………………….(2)
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47. Variation of g with Altitude
Dividing (2) by (1) we get,
m
h
M
Thus, gh is independent of the mass of the
object.
From this eqn. it is clear that the
acceleration due to gravity decreases as
altitude of the body from the earth’s
surface increases.
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48. Variation of g with Altitude
By Binomial expansion:
Since the higher powers
of h/R are neglected.
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49. Variation of g due to depth
The acceleration due to gravity on the
surface of the earth is given by:
Consider the earth as a sphere of
density ρ
Mass = Volume x Density
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50. Variation of g due to depth
Mass = Volume x Density
Mass =
………………………………………….
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(1)
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51. Variation of g due to depth
Consider a point P at the depth d below
the surface of the earth. At this point, let
the acceleration due to gravity be gd.
Distance of point P from centre of Earth
is (R – d)
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52. Variation of g due to depth
The acceleration due to gravity at point
P due to sphere of radius (R –d) is
Here, M’ is the mass of inner solid
sphere of radius (R - d)
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53. Variation of g due to depth
Mass = volume x density
……………………………………………(2)
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54. Variation of g due to depth
Dividing (2) by (1), we get,
This is the expression for the acceleration due to
gravity at a depth d below the surface of the earth.
Therefore, acceleration due to gravity decreases with
depth.
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55. Variation of g due to depth
At the centre of the earth, d = R, therefore
gd = 0
So if a body of mass m is taken to the centre of the
earth, its weight will be equal to zero (since w= mg). But
its mass will not become 0.
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56. Variation of g due to depth
g’
depth
altitude
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57. What is latitude
The latitude of a location on the Earth is
the angular distance of that location
south or north of the Equator.
Latitude of equator is 0o
Latitude of North pole is : 90o north
(+90o)
Latitude of South pole is : 90o south (90o)
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58. Variation of g due to latitude
The Earth is rotating from west to east
and the axis of rotation passes through
the poles.
Let angular velocity of earth be ω.
Every point on the surface of the earth is
moving in a circle, i.e. every point is in an
accelerated motion
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59. Variation of g due to latitude
NP-North Pole
SP-South Pole
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60. Variation of g due to latitude
Consider a body at point P on the
surface of the earth.
Let the latitude of point P be
The body at point P moves in a
circular path whose center is at Q
and radius is PQ.
PQ = r
XOP =
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61. Variation of g due to latitude
Therefore,
OPQ = (alternate
angles – transversal cutting
two parallel lines)
Centripetal acceleration
needed for a body at point P is
ar = rω2
Consider
OPQ
cos =
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62. Variation of g due to latitude
cos =
cos =
r = R cos
Therefore, ar = R cos x ω2
ar = R ω2 cos ………………. (1)
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63. Variation of g due to latitude
From OPQ, the radial component
of centripetal acceleration is
a = ar cos
= R ω2 cos cos
a
= R ω2 cos2 ……………… (2)
a
effective acceleration g’ due to
The
gravity at point P is directed towards
the centre of the earth and is given
by:
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64. Variation of g due to latitude
= g - R ω2 cos2
g’
latitude increases, cos
As
decreases, so g’ will increase.
value of g’ increases as we
The
move from the equator to the pole
due to rotation of the earth.
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65. Variation of g due to latitude
Assignment 1: Obtain an expression / value for the
acceleration due to gravity at the equator.
Assignment 2: Obtain an expression / value for the
acceleration due to gravity at the poles.
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