Time
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Time is the indefinite continued progress of existence and events that occur in apparently irreversible succession from the past through the present to the future.
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gravitation ppt srinivasa
This document outlines key concepts related to gravitation and Newton's laws of motion. It discusses Isaac Newton and his formulation of the universal law of gravitation. Some main points covered include Newton's three laws of motion, gravitational force, weight, escape velocity, Kepler's laws of planetary motion, and applications of gravitation such as keeping objects on Earth and influencing tides. The document provides an overview of fundamental principles in classical mechanics developed by Newton to describe motion and gravitational attraction.
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Johannes Kepler discovered three laws of planetary motion: 1) Planets orbit the sun in ellipses rather than perfect circles. 2) A line connecting a planet and the sun sweeps out equal areas in equal times. 3) There is a relationship between the orbital periods of planets and their distances from the sun. His discoveries helped establish that the sun, not Earth, is the center of our solar system.
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The Earth is the third planet from the Sun and the sixth largest planet in the solar system. It is not a perfect sphere, with its equator being over 27km wider than its polar diameter. The Earth has a molten iron core at its center surrounded by a viscous mantle and rigid outer crust. Beneath the crust are convection currents in the mantle that cause the movement of tectonic plates, resulting in earthquakes at their boundaries and new volcanic land at their divergent edges.
The earth
The Earth is the third planet from the Sun and the sixth largest planet in the solar system. It is not a perfect sphere, as the equator is about 24,901.55 miles in circumference and wider than the measurement between the poles. The document discusses the shape and layers of the Earth, as well as its daily rotation along its axis every 23 hours and 56 minutes and its yearly orbit around the Sun at a distance of approximately 938,900,000 km while traveling at 106,000 km per hour.
Lua
The Moon formed approximately 4.5 billion years ago from debris ejected into orbit around Earth after a collision between Earth and a Mars-sized object. In contrast, Earth has experienced ongoing geological processes like plate tectonics, erosion, and volcanism that have recycled its surface over time. The Moon has had fewer large impacts in its history than Earth and lacks an atmosphere, liquid water, plate tectonics, and an internally generated magnetic field - leading to significant differences in their surface features and evolution.
Gravity
This document discusses Newton's law of gravitation and the history of theories of gravitation, including Kepler's laws of planetary motion. It describes how Newton modified previous theories to propose that a force of gravitation exists between all masses and is proportional to the product of their masses and inversely proportional to the square of the distance between them. The document also notes how Einstein later modified Newton's law of gravitation based on his theory of relativity.
The earth
The Earth is the third planet from the Sun and the sixth largest planet in the solar system. It is not a perfect sphere, as the equator is about 24,901.55 miles in circumference and is 27km wider than the polar diameter. The document discusses the Earth's shape and size, its layers, and movements like earthquakes and volcanic eruptions.
The earth
The Earth is the third planet from the Sun and the sixth largest planet in the solar system. It is not a perfect sphere, with its equator being over 27km wider than its pole. The Earth orbits the Sun at a distance of approximately 938,900,000km along its elliptical path, rotating on its axis once every 23 hours, 56 minutes and 4.1 seconds. Earthquakes and volcanic eruptions originate from the Earth's interior layers and tectonic plate movements.
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gravitation ppt srinivasa
This document outlines key concepts related to gravitation and Newton's laws of motion. It discusses Isaac Newton and his formulation of the universal law of gravitation. Some main points covered include Newton's three laws of motion, gravitational force, weight, escape velocity, Kepler's laws of planetary motion, and applications of gravitation such as keeping objects on Earth and influencing tides. The document provides an overview of fundamental principles in classical mechanics developed by Newton to describe motion and gravitational attraction.
Kepler, Copernicus, Ptolemy, Galileo
Johannes Kepler discovered three laws of planetary motion: 1) Planets orbit the sun in ellipses rather than perfect circles. 2) A line connecting a planet and the sun sweeps out equal areas in equal times. 3) There is a relationship between the orbital periods of planets and their distances from the sun. His discoveries helped establish that the sun, not Earth, is the center of our solar system.
The earth
The Earth is the third planet from the Sun and the sixth largest planet in the solar system. It is not a perfect sphere, with its equator being over 27km wider than its polar diameter. The Earth has a molten iron core at its center surrounded by a viscous mantle and rigid outer crust. Beneath the crust are convection currents in the mantle that cause the movement of tectonic plates, resulting in earthquakes at their boundaries and new volcanic land at their divergent edges.
The earth
The Earth is the third planet from the Sun and the sixth largest planet in the solar system. It is not a perfect sphere, as the equator is about 24,901.55 miles in circumference and wider than the measurement between the poles. The document discusses the shape and layers of the Earth, as well as its daily rotation along its axis every 23 hours and 56 minutes and its yearly orbit around the Sun at a distance of approximately 938,900,000 km while traveling at 106,000 km per hour.
Lua
The Moon formed approximately 4.5 billion years ago from debris ejected into orbit around Earth after a collision between Earth and a Mars-sized object. In contrast, Earth has experienced ongoing geological processes like plate tectonics, erosion, and volcanism that have recycled its surface over time. The Moon has had fewer large impacts in its history than Earth and lacks an atmosphere, liquid water, plate tectonics, and an internally generated magnetic field - leading to significant differences in their surface features and evolution.
Gravity
This document discusses Newton's law of gravitation and the history of theories of gravitation, including Kepler's laws of planetary motion. It describes how Newton modified previous theories to propose that a force of gravitation exists between all masses and is proportional to the product of their masses and inversely proportional to the square of the distance between them. The document also notes how Einstein later modified Newton's law of gravitation based on his theory of relativity.
The earth
The Earth is the third planet from the Sun and the sixth largest planet in the solar system. It is not a perfect sphere, as the equator is about 24,901.55 miles in circumference and is 27km wider than the polar diameter. The document discusses the Earth's shape and size, its layers, and movements like earthquakes and volcanic eruptions.
The earth
The Earth is the third planet from the Sun and the sixth largest planet in the solar system. It is not a perfect sphere, with its equator being over 27km wider than its pole. The Earth orbits the Sun at a distance of approximately 938,900,000km along its elliptical path, rotating on its axis once every 23 hours, 56 minutes and 4.1 seconds. Earthquakes and volcanic eruptions originate from the Earth's interior layers and tectonic plate movements.
Earth's Motions
The document discusses the various motions of the Earth including its rotation, revolution around the sun, precession, and nutation. It explains how these motions affect seasons and tides on Earth. Additionally, it covers how the sun produces energy through nuclear fusion and transfers it to Earth through radiation, making life possible.
The Earth
The Earth is the third planet from the Sun and the sixth largest planet in the solar system. It is not a perfect sphere, with its equator being over 27km wider than its polar diameter. The Earth rotates on its axis once every 23 hours, 56 minutes and 4.1 seconds, and orbits the Sun at a distance of approximately 938,900,000 km over 365 days. It has a layered structure consisting of an inner core, outer core, mantle, and crust, and experiences regular movements in the form of earthquakes and volcanic eruptions.
The Earth
The Earth is the third planet from the sun and the sixth largest planet in the solar system. It is not a perfect sphere, with its equator being wider than its polar diameter. The Earth has layers including a crust, mantle, outer core, and inner core. The Earth rotates once every 23 hours, 56 minutes and 4.1 seconds as it orbits the sun at a speed of 106,000 km/hr along its 930,900 km circumference orbit. Earthquakes and volcanic eruptions originate from movements within the Earth's layers.
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Indian MOM(Mars Orbiter Mission), SDSC to Martian Surface #Mangalyaan #ISRO
It will be a pleasure if it helps you to understand India's Mars Mission. It was barely an opportunity for me to represent my country.I am glad to do so. Hope this will also be helpful for you. Thank you. #FeelProud #ISRO #MOM
The earth
The Earth is the third planet from the Sun and the sixth largest planet in the solar system. It is not a perfect sphere, with its equator being over 24,000 miles in circumference and wider than the distance between the poles. The Earth orbits the Sun at a distance of over 930 million kilometers and rotates on its axis once every 23 hours and 56 minutes.
The earth
The Earth is the third planet from the Sun and the sixth largest planet in the solar system. It is not a perfect sphere, with its equator circumference being about 24,901.55 miles and the equator is 27km wider than the north pole. The Earth orbits the Sun at a distance of approximately 938,900,000km, traveling at a speed of 106,000km per hour along this circumference, and rotates on its axis once every 23 hours, 56 minutes and 4.1 seconds.
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This document discusses Newton's law of universal gravitation and the development of models of the universe. It explains that Kepler analyzed Brahe's astronomical data and discovered that planets orbit the sun in ellipses. Newton then formulated his law of universal gravitation, which 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 document provides examples of applying this law and gives homework problems.
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An earthquake is caused by a sudden release of energy in the Earth's crust that creates seismic waves. The elastic rebound theory explains how rocks slowly accumulate energy from crustal movements until their strength is exceeded, causing them to break and fault. The hypocenter is where the earthquake initiates underground, while the epicenter is the point directly above on the surface. Seismic waves, including P, S, R and L waves, are detected by seismographs and used to locate the epicenter at the intersection of distance circumferences from multiple stations. Earthquakes are measured on both the Mercalli and Richter scales.
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The document describes key features of Earth, including its atmosphere, average temperature, water cycle, and magnetic field that protects from solar radiation. It also discusses Earth's rotation, which causes day and night, and its revolution around the sun, which causes the seasons. The Moon is described as Earth's only natural satellite, formed at the same time, rotating in about 29 days and orbiting Earth in about 28 days. The spheres of Earth - geosphere, hydrosphere, atmosphere, and biosphere - are also summarized.
The universe
The universe contains stars, planets, moons, asteroids, comets, and galaxies. Our solar system is made up of the Sun and objects that orbit it, including the planets. The planets can be divided into inner planets like Earth that are rocky, and outer planets like Jupiter that are gas giants. Beyond our solar system are other galaxies, including the Milky Way galaxy that contains approximately 300 billion stars and is shaped like a spiral. Scientists use measurements like distance and time to study the structure and evolution of the universe.
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Earth is the third planet from the Sun and has an average distance of 150 million km from the Sun. It revolves around the Sun due to gravitational forces and rotates on its axis, with a day lasting approximately 24 hours. Life originated on Earth around 4 billion years ago when the atmosphere lacked oxygen and the Moon was closer, with the surface covered mostly by oceans and small continents. The first photo of Earth from space was taken in 1968 by astronauts orbiting the Moon and showed Earth as a blue planet surrounded by black space.
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Space flight is important for several reasons: it allows scientists to study Earth as a planet from above the atmosphere; it permits observation of distant planets, stars, and galaxies without atmospheric filtering; and it enables direct sampling of other worlds. Space flight also provides a microgravity environment for investigating fundamental states of matter and forces.
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The universe contains over 100 billion galaxies scattered throughout over 10 billion light years of space. It formed around 13.8 billion years ago in an event known as the Big Bang, in which all matter, energy, space and time exploded into existence from a single point. The universe has been expanding ever since, with the observable portion extending 46 billion light years from Earth due to the ongoing expansion over billions of years.
The earth
The Earth is the third planet from the Sun and the sixth largest planet in the solar system. It is not a perfect sphere, with its equator being over 27km wider than its polar diameter. The Earth rotates on its axis once every 23 hours, 56 minutes and 4.1 seconds, and orbits the Sun at a distance of approximately 938,900,000km along its circumference at a speed of 106,000km per hour. It has four main layers - the inner and outer core, mantle, and crust - and earthquakes and volcanic eruptions originate from movements within these layers.
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The distance between the sun and earth is 150,000,000,000 metres. Light travels at 300,000 km per second, and light year is the distance light travels in one year which is about 9.5x1015 metres. The document also provides comparative sizes and masses of planets in our solar system.
Space
Space is not empty according to modern physics. Newton saw space and time as absolute and space as rigid, while Einstein saw them as flexible and relative. Einstein's theory of general relativity established that massive objects curve space and time, and that the speed of light in a vacuum is constant regardless of the motion of its source. Understanding space can provide insights into the origin and workings of the universe.
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The Earth is the third planet from the Sun and the sixth largest planet in the solar system. It is not a perfect sphere, as the equator is about 24,901.55 miles in circumference and is 27km wider than the polar diameter. The Earth rotates on its axis once every 23 hours, 56 minutes and 4.1 seconds. The document discusses the origins of earthquakes and volcanic eruptions.
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The earth
The Earth is the third planet from the Sun and the sixth largest planet in the solar system. It is not a perfect sphere, with its equator being over 27km wider than its polar diameter. The Earth consists of layers including a crust, mantle, lithosphere, and core. It rotates on its axis once every 23 hours and 56 minutes while orbiting the Sun at a speed of over 106,000 km/hr along its nearly 940 million km circumference.
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El documento resume aspectos de la vida cotidiana en Buenos Aires en 1816, el año de la independencia de Argentina. Describe las características de las casas coloniales, las costumbres sociales como las tertulias y reuniones en patios, la vestimenta formal de la época, los estilos musicales populares como el tango, minué y folklore, y la composición de la Primera Junta de Gobierno.
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The Earth
The Earth is the third planet from the Sun and the sixth largest planet in the solar system. It is not a perfect sphere, with its equator being over 27km wider than its polar diameter. The Earth rotates on its axis once every 23 hours, 56 minutes and 4.1 seconds, and orbits the Sun at a distance of approximately 938,900,000 km over 365 days. It has a layered structure consisting of an inner core, outer core, mantle, and crust, and experiences regular movements in the form of earthquakes and volcanic eruptions.
The Earth
The Earth is the third planet from the sun and the sixth largest planet in the solar system. It is not a perfect sphere, with its equator being wider than its polar diameter. The Earth has layers including a crust, mantle, outer core, and inner core. The Earth rotates once every 23 hours, 56 minutes and 4.1 seconds as it orbits the sun at a speed of 106,000 km/hr along its 930,900 km circumference orbit. Earthquakes and volcanic eruptions originate from movements within the Earth's layers.
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The document summarizes the formation and components of the Milky Way galaxy and solar system. It describes how the universe was formed in the Big Bang around 13.8 billion years ago. It then explains how 5 billion years ago, the solar system formed from a cloud of gas and dust that collapsed into the Sun and planets. Finally, it provides brief descriptions of the planets, moons, and other components that make up our solar system.
Indian MOM(Mars Orbiter Mission), SDSC to Martian Surface #Mangalyaan #ISRO
It will be a pleasure if it helps you to understand India's Mars Mission. It was barely an opportunity for me to represent my country.I am glad to do so. Hope this will also be helpful for you. Thank you. #FeelProud #ISRO #MOM
The earth
The Earth is the third planet from the Sun and the sixth largest planet in the solar system. It is not a perfect sphere, with its equator being over 24,000 miles in circumference and wider than the distance between the poles. The Earth orbits the Sun at a distance of over 930 million kilometers and rotates on its axis once every 23 hours and 56 minutes.
The earth
The Earth is the third planet from the Sun and the sixth largest planet in the solar system. It is not a perfect sphere, with its equator circumference being about 24,901.55 miles and the equator is 27km wider than the north pole. The Earth orbits the Sun at a distance of approximately 938,900,000km, traveling at a speed of 106,000km per hour along this circumference, and rotates on its axis once every 23 hours, 56 minutes and 4.1 seconds.
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This document discusses Newton's law of universal gravitation and the development of models of the universe. It explains that Kepler analyzed Brahe's astronomical data and discovered that planets orbit the sun in ellipses. Newton then formulated his law of universal gravitation, which 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 document provides examples of applying this law and gives homework problems.
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An earthquake is caused by a sudden release of energy in the Earth's crust that creates seismic waves. The elastic rebound theory explains how rocks slowly accumulate energy from crustal movements until their strength is exceeded, causing them to break and fault. The hypocenter is where the earthquake initiates underground, while the epicenter is the point directly above on the surface. Seismic waves, including P, S, R and L waves, are detected by seismographs and used to locate the epicenter at the intersection of distance circumferences from multiple stations. Earthquakes are measured on both the Mercalli and Richter scales.
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The document describes key features of Earth, including its atmosphere, average temperature, water cycle, and magnetic field that protects from solar radiation. It also discusses Earth's rotation, which causes day and night, and its revolution around the sun, which causes the seasons. The Moon is described as Earth's only natural satellite, formed at the same time, rotating in about 29 days and orbiting Earth in about 28 days. The spheres of Earth - geosphere, hydrosphere, atmosphere, and biosphere - are also summarized.
The universe
The universe contains stars, planets, moons, asteroids, comets, and galaxies. Our solar system is made up of the Sun and objects that orbit it, including the planets. The planets can be divided into inner planets like Earth that are rocky, and outer planets like Jupiter that are gas giants. Beyond our solar system are other galaxies, including the Milky Way galaxy that contains approximately 300 billion stars and is shaped like a spiral. Scientists use measurements like distance and time to study the structure and evolution of the universe.
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Earth is the third planet from the Sun and has an average distance of 150 million km from the Sun. It revolves around the Sun due to gravitational forces and rotates on its axis, with a day lasting approximately 24 hours. Life originated on Earth around 4 billion years ago when the atmosphere lacked oxygen and the Moon was closer, with the surface covered mostly by oceans and small continents. The first photo of Earth from space was taken in 1968 by astronauts orbiting the Moon and showed Earth as a blue planet surrounded by black space.
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Universe
The universe contains over 100 billion galaxies scattered throughout over 10 billion light years of space. It formed around 13.8 billion years ago in an event known as the Big Bang, in which all matter, energy, space and time exploded into existence from a single point. The universe has been expanding ever since, with the observable portion extending 46 billion light years from Earth due to the ongoing expansion over billions of years.
The earth
The Earth is the third planet from the Sun and the sixth largest planet in the solar system. It is not a perfect sphere, with its equator being over 27km wider than its polar diameter. The Earth rotates on its axis once every 23 hours, 56 minutes and 4.1 seconds, and orbits the Sun at a distance of approximately 938,900,000km along its circumference at a speed of 106,000km per hour. It has four main layers - the inner and outer core, mantle, and crust - and earthquakes and volcanic eruptions originate from movements within these layers.
social explore
The distance between the sun and earth is 150,000,000,000 metres. Light travels at 300,000 km per second, and light year is the distance light travels in one year which is about 9.5x1015 metres. The document also provides comparative sizes and masses of planets in our solar system.
Space
Space is not empty according to modern physics. Newton saw space and time as absolute and space as rigid, while Einstein saw them as flexible and relative. Einstein's theory of general relativity established that massive objects curve space and time, and that the speed of light in a vacuum is constant regardless of the motion of its source. Understanding space can provide insights into the origin and workings of the universe.
The earth
The Earth is the third planet from the Sun and the sixth largest planet in the solar system. It is not a perfect sphere, as the equator is about 24,901.55 miles in circumference and is 27km wider than the polar diameter. The Earth rotates on its axis once every 23 hours, 56 minutes and 4.1 seconds. The document discusses the origins of earthquakes and volcanic eruptions.
Izabela's Mars One Project
The Mars One communication system uses satellites to enable communication between Mars and Earth. A Mars-stationary satellite remains fixed above one location on Mars to allow near 24/7 communication. A second satellite is placed around the sun to provide coverage when the sun is directly between Mars and Earth, which occurs every 26 months for about six weeks. Due to the distance between Mars and Earth, there is a communication delay of 3 to 22 minutes each way. This delay prevents real-time communication like phone calls.
The earth
The Earth is the third planet from the Sun and the sixth largest planet in the solar system. It is not a perfect sphere, with its equator being over 27km wider than its polar diameter. The Earth consists of layers including a crust, mantle, lithosphere, and core. It rotates on its axis once every 23 hours and 56 minutes while orbiting the Sun at a speed of over 106,000 km/hr along its nearly 940 million km circumference.
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The document discusses three physical models that attempt to explain time travel: classical mechanics, relativistic mechanics, and quantum mechanics. It describes Einstein's theory of relativity which adds time as a fourth dimension and shows how time is relative to velocity and acceleration. The document also considers whether time travel is possible based on theories of gravity affecting the flow of time and the twin paradox, but concludes it is unclear if traveling back in time could be achieved.
Dozier presentation
An artist painting an oil painting illustrates quantum atom theory and the Heisenberg uncertainty principle, as the artist is manipulating subatomic particles but is uncertain of the final outcome. Every movement by the artist starts at the quantum level and has uncertainty in momentum and position. Recent experiments have challenged Heisenberg's uncertainty principle by measuring subatomic particles without disturbing them. Quantum entanglement and spooky actions from a distance connect particles over vast distances instantly, and may one day allow quantum teleportation and encryption.
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Astronomy by quran and hadist and scientific evidence
The document discusses scientific evidence that supports the propositions in the Quran that the sun moves and the earth is motionless:
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2) The "geodetic wrap" effect and experiments with the "trigger effect" technology prove the earth is motionless at the center of the universe.
3) Experiments controlling the magnetic field with Helmholtz coils show Earth's magnetic field is stable, indicating it is not subject to major changes from earth's movement.
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1) The document discusses Newton's laws of motion and the development of Newton's law of gravity. It describes how Newton imagined the force that causes apples to fall on Earth also reaches the moon.
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3) Newton's laws were incredibly successful and his law of gravity was not revised or suspected to be wrong for 150 years after he developed it.
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C04011 03 1925
This document discusses theories of interstellar communication and time travel. It covers the following key points:
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2. Wormhole theory proposes that wormholes could connect distant regions of space and act as shortcuts for interstellar travel or travel between different points in time. However, generating human-sized wormholes requires energy levels far beyond today's capabilities.
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The Amazing Speed of Light Across the Universe.pdf
But what is the speed of light, and how does it affect our understanding of the universe?
What Is the Speed of Light?
The speed of light is a physical constant, denoted by the symbol "c", which is approximately 299,792,458 meters per second, or about 670,616,629 miles per hour. It is the speed at which electromagnetic radiation, such as light, travels through a vacuum. The speed of light is considered to be an absolute physical constant because it is the same in all inertial reference frames and is not affected by the motion
How Fast Does Light Travel?
The speed of light is a physical constant that is the same in all inertial reference frames and is not affected by the observer's motion or the light's source. It is approximately 299,792,458 meters per second or about 670,616,629 miles per hour.
To give you an idea of how fast this is, consider that it would take light about 8 minutes and 20 seconds to travel from the Sun to the Earth, It would take light about 4 years to travel from the nearest star beyond the Sun, Proxima Centauri, which is about 25 trillion miles (4.24 light-years) away.
What Are the Implications of the Speed of Light?
The speed of light has many important implications in a variety of fields, including astronomy, physics, and engineering. Some of the key implications of the speed of light are:
The speed of light sets a fundamental limit on the speed at which information and signals can be transmitted. This means that nothing with mass can travel faster than the speed of light.
The speed of light has important implications for the study of celestial objects and the structure of the universe. For example, the finite speed of light means that when we look at distant objects in the universe, we are looking back in time.
The speed of light is an important factor in the theory of relativity, which explains how the laws of physics behave in different reference frames. The theory of relativity predicts that time and space are relative and that the speed of light is the same in all inertial reference frames.
The speed of light has practical applications in a variety of fields, including telecommunications, navigation, and satellite technology. For example, the time it takes for a signal to travel from a satellite to the Earth is used to calculate the distance between the satellite and the Earth.
Expansion of the Universe
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Write up Final
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2) By solving the resulting differential equation numerically, the model can determine the impact time and velocity of a satellite. This allows estimates of the damage caused and time for evacuation if the satellite were to impact a populated area.
3) The document provides an example application of the model to Sputnik 1 and graphs the results, showing a impact time of about 5.5 minutes and velocity of 47 m/s.
Gravitation (Class XI Brief)
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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MODERN-PHYSICS-Franks.pdf
The document discusses the history and nature of theories of light. It describes early theories including Newton's particle theory and Huygens' wave theory. It then explains Maxwell's electromagnetic theory and Einstein's quantum theory of light, which unified wave and particle properties. The development of theories has been driven by experiments and mathematics. Today's accepted theory is the quantum theory of light, which has revolutionized understanding and technology development like lasers and optical devices.
What is the Speed of Light !!!!.pdf
Chapters
Reminders: light
speed of light in a vacuum
A brief historical reminder of the speed of light
Invariance of the speed of light in a vacuum
Influence of the propagation medium
Speed or celerity?
Speed, distance traveled, and duration
Relations including the speed of light
Faster than light?
Speed of light: did you know?
Reminders: light
Light is an electromagnetic wave, consisting of a magnetic field and an electric field oscillating perpendicular to each other in a plane perpendicular to the direction of propagation of the light wave. In a vacuum, light travels in a straight line at the speed of light noted c.
speed of light in a vacuum
Exact value
The exact value of the speed of light was fixed in 1983 by the Bureau of Weights and Measures at c = 299 792 458 m/s or c = 2.99792458 x 10 8 m/s, using the units of the international system. It can also be expressed in kilometers per hour by multiplying the value in m/s by 3.6: c = 1,079,252,848.8 km/h or c = 1.0792528488 x 10 9 km/h. This value, which represents a fundamental constant of physics, can be used for calculations requiring great precision. It is also used to define the meter in the international system of units: one meter corresponds to the length traveled in a vacuum by light for a duration of 1/299,792,458 seconds.
A brief historical reminder of the speed of light
The first conception concerning light suppose that it can be either present in a space, or absent: the light would therefore be instantaneous. The Arab scholar Alhazen (965-1039) was interested in optics and wrote reference treatises. He is the first to have the intuition that the appearance of light is not instantaneous, that it has a speed of propagation, but he cannot prove it.
Galileo (1564-1039) tries to measure the propagation time of light between two hills using two people a few kilometers apart and equipped with clocks. He fails to measure the speed of light (which, in the context of this experiment, takes 10 -5 seconds to travel the previously defined distance, not measurable for the time) and deduces from the failure of this experiment that the speed of propagation of light is very high.
Cassini (1625-1712) speculated that the irregularity in the movement of Io, a satellite of Jupiter, could come from a delay in the arrival of light from the satellite, "such that it takes 10 or 11 minutes for it travels a distance equal to the radius of the Earth's orbit". Römer (1644-1710) explains the discrepancy between the eclipses of Io (a satellite of Jupiter) and Cassini's predictions by assuming that light has a speed of propagation. It is the first to give an order of magnitude of the speed of light.
Bradley (1693-1762) confirms Römer's hypothesis and proposes a first estimate of the speed of light at approximately 10188 times that of the rotation of the Earth around the Sun, the latter being however poorly known. His discovery is linked to the aberration of light,
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Gravity
This document discusses the differences between mass and weight, Newton and Einstein's theories of gravity, and how gravity works. According to Newton, gravity is a force that attracts objects with mass. Einstein viewed gravity as the warping of spacetime by massive objects. Under Einstein's theory, objects follow curved paths in spacetime rather than experiencing a gravitational force.
Cosmic Histories and human perspectives: A journey through time and space
The document discusses the evolution of human understanding of the universe through history. It begins with early astronomy among ancient civilizations like Babylonians, Greeks, Indians, Egyptians and Chinese. It then outlines major developments including Copernicus' heliocentric model, Kepler's laws, Galileo's observations supporting Copernicus, Newton's laws of motion and gravity, and Einstein's theory of general relativity. The document also summarizes modern cosmological concepts like the expansion of the universe observed by Hubble, the hot dense early universe, formation of light elements in Big Bang nucleosynthesis, cosmic microwave background radiation, and evolution of the universe from the dark ages to the present epoch.
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Cosmology is the study of the origin and evolution of the universe. Observational evidence shows the universe is expanding, with more distant galaxies receding faster. The cosmological principle states the universe appears homogeneous and isotropic at large scales. Matter in the universe includes baryons like protons and neutrons, photons that make up radiation, neutrinos, and non-baryonic dark matter. The expansion of the universe is governed by Friedman equations involving the scale factor and density of the universe. Simple cosmological models can be constructed assuming the universe is filled with either pressureless matter or radiation.
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The Seven Basic Tools of Quality is a designation given to a fixed set of graphical techniques identified as being most helpful in troubleshooting issues related to quality.They are called basic because they are suitable for people with little formal training in statistics and because they can be used to solve the vast majority of quality-related issues.
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The document provides an overview of search engine optimization (SEO). It defines SEO as improving the volume and quality of traffic from organic search results. It discusses the current state of search and market share of different search engines. It also outlines the differences between organic and paid search results. The document then discusses how search engines work, why SEO is important, factors that influence search engine rankings, and provides tips for basic on-site and off-site SEO optimization techniques.
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9
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Time
- 1. Time
- 2. Overview Concept of Time Parameters that relates to Time Impact of parameters in Time.
- 3. Concept of Time ➲ Time is a real phenomenon a continuous change through which we live. Time becomes evident through motion; sunrise sunsets, night and day, the. ... Other important aspect of time is presence of motion of particles like photon, the motion at the. atomic and subatomic level. ➲ Time is an observed phenomenon, by means of which human beings sense and record changes in the environment and in the universe.
- 4. Parameters that relates to Time ➲ Velocity & Space ➲ Inhabitance ➲ Gravitational Forces of Celestial Bodies
- 5. Impact of Velocity ➲ Speed of Light = 3+E8 m/s ➲ Diameter of earth = 12,742km ➲ Circumference of Earth = 40,030km Eg.: A train at the speed of light moves at 0 friction space at the path of the perimeter of earth at 7º to earth's equator, which gives the exact count of 7 times per second i.e moving around the earth 7 times per second.
- 7. Einstein's most famous equation e=mc² At this state of motion the mass tremendously increases and finally the mass vanishes like a photon and neglects the impact of time. For a one day of journey in the train will move us to the future i.e the mass moving along inside the train in the speed of light has came over the effect of time. So at the end of journey we might be moved to future as other would be at impact of time. 1 hour inside the train = 600 hours (approx.) outside the world
- 8. Impact of Inhabitance Biological clock of brain Factors that makes impact on time Interest Concentration Involvement All these three factors are major for a saint to over come?
- 9. Gravity force of Celestial Bodies Major axisMajor axis
- 10. Time is just a parameter for a person who is busy with work. Time is a important factor for all person who fights for life. Time is dependent on persons Don't waste time when available!!!
- 11. Thank You For Your Attention