This document discusses rotational motion of rigid bodies and satellites. It defines rigid bodies and rotational motion, and describes concepts like moment of inertia, kinetic energy of rotating bodies, and gravitational force. It then discusses different types of satellites like geo-stationary and polar satellites, and their uses which include weather monitoring, remote sensing, communication, and military applications.
Tis ppt gives u a brief glance on the following topics:
Escape Speed
Earth Satellites
Geostationary And Polar Satellites
Weightlessness
If u want to download the ppt mail me to raviteja711@gmail.com
Tis ppt gives u a brief glance on the following topics:
Escape Speed
Earth Satellites
Geostationary And Polar Satellites
Weightlessness
If u want to download the ppt mail me to raviteja711@gmail.com
Geodetic Astronomy - MOTION IN THE HEAVENS - EARTH, SUN AND STARSAhmed Nassar
Geodetic Astronomy
MOTION IN THE HEAVENS
EARTH, SUN AND STARS
Motion of Earth
Earth’s Rotation
Earth’s Revolution
Motion of Sun
Equinoxes
Solstices
Motion of Stars
Proper Motion
Transverse Velocity
Radial Velocity
A gyroscope, not to be confused with gyrocompass, is a spinning wheel mounted on gimbal so that the wheel's axis is free to orient itself in any way. When it is spun up to speed with its axis pointing in some direction, due to the law of conservation of angular momentum, such a wheel will normally maintain its original orientation to a fixed point in outer space (not to a fixed point on 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.
Geodetic Astronomy - MOTION IN THE HEAVENS - EARTH, SUN AND STARSAhmed Nassar
Geodetic Astronomy
MOTION IN THE HEAVENS
EARTH, SUN AND STARS
Motion of Earth
Earth’s Rotation
Earth’s Revolution
Motion of Sun
Equinoxes
Solstices
Motion of Stars
Proper Motion
Transverse Velocity
Radial Velocity
A gyroscope, not to be confused with gyrocompass, is a spinning wheel mounted on gimbal so that the wheel's axis is free to orient itself in any way. When it is spun up to speed with its axis pointing in some direction, due to the law of conservation of angular momentum, such a wheel will normally maintain its original orientation to a fixed point in outer space (not to a fixed point on 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.
SUMMARY OF CHAPTER:-
Definition of Gravitation
Acceleration Due to Gravity
Variation Of “G” With Respect to Height And Depth
Escape Velocity
Orbital Velocity
Gravitational Potential
Time period of a Satellite
Height of Satellite
Binding Energy
Various Types of Satellite
Kepler’s Law of Planetary motion
Contact: Facebook URL: fb.com/sajidhasanrawnak
This Slides will answer the following Questions-
What is Orbit?
Different types of orbit used in Satellite System? Explain each of them in brief.
Familiarization of different orbital parameters defining the satellite orbit with detail description.
Basic principles of orbiting satellites - Kepler’s Laws
What is eccentricity? How it is characterized the shape of an orbit?
What is orbital period? Derivation of orbital period. Explain how eccentricity and flattening plays a vital role to visualized the shape of earth?
What is Injection Velocity? How it affects the Resulting Satellite Trajectories?
Conditions required to become a geostationary satellite?
Slant Range.
Line-of-sight distance between two satellites.
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.
Week 3 OverviewLast week, we covered multiple forces acting on.docxmelbruce90096
Week 3 Overview
Last week, we covered multiple forces acting on an object. This week we will cover motion in two dimensions, inclined planes, circular motion, and rotation.
Forces in Two Dimensions (1 of 2)
So far you have dealt with single forces acting on a body or more than two forces that act parallel to each other. But in real life situations more than one force may act on a body. How are Newton's laws applied to such cases? We will restrict the forces to two dimensions.
Since force and acceleration are vectors, Newton's law can be applied independently to the X and Y-axes of a coordinate system. For a given problem you can choose a suitable coordinate system. But once a coordinate system is chosen, we have to stick with it for that problem. The example that follows shows how to find the acceleration of a body when two forces act on it at right angles to each other.
Forces in Two Dimensions (2 of 2)
To find the resultant acceleration we draw an arrow OA of length 3 units along the X-axis and then an arrow AB of length 4 units along the Y-axis. The resultant acceleration is the arrow OB with the length of 5 units. Therefore, the acceleration is 5 m/s2 in the direction of OB. Also when you measure the angle AOB with a protractor, we find it to be 53°.
The acceleration caused by the two forces is 5 m/s2 at an angle of 53°.
Uniform Circular Motion
When an object travels in a circular path at a constant speed, its motion is referred to as uniform circular motion, and the object is accelerated towards the center of the circle. If the radius of the circular path is r, the magnitude of this acceleration is ac = v2 / r, where v is its speed and ac is called the centripetal acceleration. A centripetal force is responsible for the centripetal acceleration, which constantly pulls the object towards the center of the circular path. There cannot be any circular motion without a centripetal force.
Banking
When there is a sharp turn in the road or when a turn has to be taken at a high speed as in a racetrack, the outer part of the road or the track is raised from the inner part of the track. This is called banking. It provides additional centripetal force to a turning vehicle so that it doesn't skid.
The angle of banking is kept just right so that it provides all the centripetal force required and a motorist does not have to depend on the friction force at all.
Inclined Planes
Forces on an Inclined Plane
The inclined plane is a device that reduces the force needed to lift objects. Consider the forces acting on a block on an inclined surface. The inclined surface exerts a normal force FN on the block that is perpendicular to the incline. The force of gravity, FG, points downward. If there is no friction, the net force, Fnet, acting on the block is the resultant of FN and FG. By Newton's second law the net force must point down the incline because the block moves only along the incline and not perpendicular to it.
The vector triangle shows .
Remember it's just a start for class 20 students. Just a way to declare hot to teach students of class by using the scope of ICT . It declares the scope of ICT in the field of education.
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
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Saudi Arabia stands as a titan in the global energy landscape, renowned for its abundant oil and gas resources. It's the largest exporter of petroleum and holds some of the world's most significant reserves. Let's delve into the top 10 oil and gas projects shaping Saudi Arabia's energy future in 2024.
Using recycled concrete aggregates (RCA) for pavements is crucial to achieving sustainability. Implementing RCA for new pavement can minimize carbon footprint, conserve natural resources, reduce harmful emissions, and lower life cycle costs. Compared to natural aggregate (NA), RCA pavement has fewer comprehensive studies and sustainability assessments.
About
Indigenized remote control interface card suitable for MAFI system CCR equipment. Compatible for IDM8000 CCR. Backplane mounted serial and TCP/Ethernet communication module for CCR remote access. IDM 8000 CCR remote control on serial and TCP protocol.
• Remote control: Parallel or serial interface.
• Compatible with MAFI CCR system.
• Compatible with IDM8000 CCR.
• Compatible with Backplane mount serial communication.
• Compatible with commercial and Defence aviation CCR system.
• Remote control system for accessing CCR and allied system over serial or TCP.
• Indigenized local Support/presence in India.
• Easy in configuration using DIP switches.
Technical Specifications
Indigenized remote control interface card suitable for MAFI system CCR equipment. Compatible for IDM8000 CCR. Backplane mounted serial and TCP/Ethernet communication module for CCR remote access. IDM 8000 CCR remote control on serial and TCP protocol.
Key Features
Indigenized remote control interface card suitable for MAFI system CCR equipment. Compatible for IDM8000 CCR. Backplane mounted serial and TCP/Ethernet communication module for CCR remote access. IDM 8000 CCR remote control on serial and TCP protocol.
• Remote control: Parallel or serial interface
• Compatible with MAFI CCR system
• Copatiable with IDM8000 CCR
• Compatible with Backplane mount serial communication.
• Compatible with commercial and Defence aviation CCR system.
• Remote control system for accessing CCR and allied system over serial or TCP.
• Indigenized local Support/presence in India.
Application
• Remote control: Parallel or serial interface.
• Compatible with MAFI CCR system.
• Compatible with IDM8000 CCR.
• Compatible with Backplane mount serial communication.
• Compatible with commercial and Defence aviation CCR system.
• Remote control system for accessing CCR and allied system over serial or TCP.
• Indigenized local Support/presence in India.
• Easy in configuration using DIP switches.
Sachpazis:Terzaghi Bearing Capacity Estimation in simple terms with Calculati...Dr.Costas Sachpazis
Terzaghi's soil bearing capacity theory, developed by Karl Terzaghi, is a fundamental principle in geotechnical engineering used to determine the bearing capacity of shallow foundations. This theory provides a method to calculate the ultimate bearing capacity of soil, which is the maximum load per unit area that the soil can support without undergoing shear failure. The Calculation HTML Code included.
Planning Of Procurement o different goods and services
Unit 4 DYNAMICS – II
1. Faculty : Engineering
Department :Telecommunication
Engineering
Subject: Engineering Physics SEM I
LECTURER :AHMEDLECTURER :AHMEDLECTURER :AHMEDLECTURER :AHMED ABDIREHMANABDIREHMANABDIREHMANABDIREHMAN
Head of the department of telecommunication
engineering
Engineering
2. Rotational Motion of Rigid Bodies
UNIT -4 :DYNAMICS – II
Rotational Motion of Rigid Bodies
Gravitation
Satellites
3. 4.1 ROTATIONAL4.1 ROTATIONAL4.1 ROTATIONAL4.1 ROTATIONAL MOTION OF RIGID BODIESMOTION OF RIGID BODIESMOTION OF RIGID BODIESMOTION OF RIGID BODIES
Rigid body
A rigid body may be defined as that body which does not undergo any
change in its shape or size due to the application of force.
Rotational motion.
When the body rotates about a fixed line (axis of rotation), its motion isWhen the body rotates about a fixed line (axis of rotation), its motion is
known as rotator motion.
The axis of rotation may lie within the body or outside the body. When a
body is in rotational motion about an axis, all the particles present in
the body will have same angular velocity, but different linear velocities.
The values of the linear velocities of these particles depend on the
distance of the particles from the axis of rotation, since v = r w
4. Moment of Inertia of a particleMoment of Inertia of a particleMoment of Inertia of a particleMoment of Inertia of a particle
The inability of a body to change its state on its own, without the help of
external force is termed as inertia.
The moment of inertia of a particle about an axis is equal to the product of
the mass of the particle and square of its distance from the axis.The S.I.
unit for moment of inertia is kg m2.
5. Moment of Inertia of a rigid bodyMoment of Inertia of a rigid bodyMoment of Inertia of a rigid bodyMoment of Inertia of a rigid body
Similarly Moment of inertia of a body is its inability to change by itself its state of rest or of
uniform rotator motion about an axis.
6.
7. Expression for Kinetic Energy of a Rigid body rotating about an
axis:
Consider a rigid body rotating about a fixed axis , Let m1 , m2 , m3 ,….. ... etc., be the
masses of the particles situated at distances. r1 , r2 , r3 , ...... etc., from the fixed axis.
All the particles rotate with the same angular velocity w. But the linear velocities of the
particles are different.
8.
9.
10.
11. 4.2 GRAVITATION4.2 GRAVITATION4.2 GRAVITATION4.2 GRAVITATION
Newton’s laws of Gravitation
Law 1 :Any two particles of matter attract each other with a force
Law 2 :The force of attraction between any two objects is
i. directly proportional to the product of the masses
ii. inversely proportional to the square of the distance
between them.
If m1 , m2 are masses of two particles, separated by a distance‘d’ then
the force of attraction between the particles,
12. Acceleration due to gravityAcceleration due to gravityAcceleration due to gravityAcceleration due to gravity
The acceleration produced in a body on account of the force of gravity
is called acceleration due to gravity. It is denoted by‘g’.At a given
place, the value of‘g’ is the same for all bodies irrespective of their
masses. It differs from place to place on the surface of the Earth. It also
varies with altitude and depth
The value of g at sea-level and at a latitude of 45° is taken as the
standard (i.e) g = 9.81 m s–2.standard (i.e) g = 9.81 m s–2.
13.
14.
15. WeightlessnessWeightlessnessWeightlessnessWeightlessness
Consider the astronaut standing on the ground. He exerts a force
(his weight) on the ground. At the same time, the ground exerts an
equal and opposite force of reaction on the astronaut. Due to this
force of action, he has a feeling of weight.
When the astronaut is in an orbiting satellite, both the satellite and
astronaut have the same acceleration towards the centre of theastronaut have the same acceleration towards the centre of the
earth. Hence, the astronaut does not exert any force on the floor of
the satellite. So, the floor of the satellite also does not exert any
force of action on the astronaut. As there is no reaction, the
astronaut has a feeling of weightlessness.
16. 4.3 SATELLITES4.3 SATELLITES4.3 SATELLITES4.3 SATELLITES
A body moving in an orbit around another bigger body is called a
satellite.A body that moves around a planet is called a satellite.
The objects that are moving in orbit by nature itself around a planet
are called natural satellites. For example, moon is the natural
satellite for the earth.The earth is a satellite for the sun.
Man also has placed artificially some satellites to move in orbit
around the desired planets. These satellites are called artificialaround the desired planets. These satellites are called artificial
satellite.
The artificial satellites are carried by rockets to the predetermined
height, a few hundred kilometers above the surface of the earth.
The artificial satellites are broadly classified as earth resources
satellites, meteorological satellites and satellites carrying microwave
sensors.
17. Escape velocity and Orbital velocityEscape velocity and Orbital velocityEscape velocity and Orbital velocityEscape velocity and Orbital velocity
Escape velocity (Ve):
When a body is thrown vertically
upwards, it will return to the
earth’s surface after attaining
certain height. If the velocity of
projection is increased, the height
attained by the body becomes
greater and then the body returns
to the earth. This is due to the
Orbital velocity (Vo)
In order to put a satellite into
the orbit around the earth,
the satellite must be
projected to the particular
height and then it must be
turned in a direction
perpendicular to the line
from the centre of the earthto the earth. This is due to the
gravitational force of attraction of
the earth. If the body is to be
projected with a particular greater
velocity, the body escapes from the
gravitational pull so that it never
returns to the earth. This velocity of
projection is called escape velocity,
it is different for different planets.
from the centre of the earth
so that it moves in an orbit
around the earth.
The velocity of the satellite
along its orbit around the
earth is called orbital
velocity.
18.
19.
20.
21.
22.
23.
24. GeoGeoGeoGeo –––– Stationary SatelliteStationary SatelliteStationary SatelliteStationary Satellite
A geo-stationary satellite is a particular type used in television
and telephone communications.A number of communication
satellites, which appear to remain in fixed position at a height of
36,000 km above the equator, are called synchronous satellites or
geostationary satellites. In this orbit, the satellite takes 24 hours
for revolving round the earth once
Some television programmers or events occurring in otherSome television programmers or events occurring in other
countries are often transmitted live with the help of these
satellites.
As the geostationary satellite can‘see’ only one-third of the
earth’s surface, atleast three such satellites are required to cover
the entire globe.
25. Polar SatellitesPolar SatellitesPolar SatellitesPolar Satellites
The polar satellites revolve around the earth in a north-south orbit
passing over the poles as the earth spins about its north-south axis.
The Polar satellites positioned nearly 500 to 800 km above the earth
travels from pole to pole in 102 minutes. The polar orbit remains
fixed in space as the earth rotates inside the orbit. As a result, mostfixed in space as the earth rotates inside the orbit. As a result, most
of the earth’s surface crosses the satellite in a polar orbit. Excellent
coverage of the earth is possible with this polar orbit.
The polar satellites are used for mapping and surveying.
26. Uses of Artificial SatellitesUses of Artificial SatellitesUses of Artificial SatellitesUses of Artificial Satellites
The artificial satellites are launched for many purposes by
different countries.The important uses of artificial
satellite are
i. Collection of scientific data
ii.Weather monitoring
iii. Military Spyingiii. Military Spying
iv. Remote sensing
v. Communication purpose – the satellite receives
microwaves andTV signals from the earth and amplifies
them and transmits them back to various stations on
the earth.