PP16_-_Universal_Gravitation.ppt
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1) Isaac Newton proposed a law of universal gravitation in 1666 that states any two objects attract each other with a gravitational force proportional to the product of their masses and inversely proportional to the square of the distance between them. 2) The law explains that gravity is what keeps planets in orbit around the sun and the moon in orbit around Earth. 3) Henry Cavendish experimentally determined the proportionality constant G in 1798, known as the gravitational constant, which is equal to 6.67 x 10-11 N m2 / kg2.
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Universal_Gravitation.ppt
Newton proposed 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. This law explained the force keeping the planets in orbit around the sun and the moon orbiting the Earth. Later experiments determined the proportionality constant in Newton's equation.
Law of Universal Gravitation
1) Isaac Newton proposed a law of universal gravitation in 1666 stating that any two objects attract each other with a gravitational force proportional to the product of their masses and inversely proportional to the square of the distance between them.
2) The law explained the force keeping planets in orbit around the Sun and the Moon orbiting the Earth.
3) In 1798, Henry Cavendish experimentally determined the proportionality constant G in Newton's law of universal gravitation.
Universal gravitation arun
1) Isaac Newton formulated his law of universal gravitation in 1666, which states that any two objects attract each other with a force proportional to the product of their masses and inversely proportional to the square of the distance between them.
2) Henry Cavendish experimentally determined the proportionality constant G in 1798, which is equal to 6.67 x 10-11 N m2 / kg2.
3) Newton's law of universal gravitation explains why objects like the moon orbit the earth rather than falling straight down, and suggests that the force of gravity is universal across all masses in the universe.
Digital text
1) Gravitation is the fundamental force of attraction between objects with mass. Newton discovered that gravitation causes objects to be pulled toward each other, with a force that is directly proportional to their masses and inversely proportional to the square of the distance between them.
2) Newton formulated his universal law of gravitation after observing an apple fall from a tree and realizing that the same force must cause objects on Earth and celestial bodies like the moon to fall or orbit.
3) Newton's theory explained phenomena that were previously not understood, like why objects in orbit do not fly off into space, and it provided an understanding of gravity that lasted over two centuries until Einstein improved on the theory with his theory of general relativity.
Gravitation theory
1) Gravity is a natural phenomenon that causes all objects with mass to attract each other. Modern physics describes gravitation through Einstein's general theory of relativity, which views gravity as a distortion of spacetime by massive objects.
2) Isaac Newton formulated the law of universal gravitation, which 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) Newton's theory accounted for the motions of celestial bodies and dominated scientists' views of the physical universe for three centuries, until Einstein's general relativity resolved some discrepancies like Mercury's orbit.
Newtons Law of Universal Gravitation.ppt
Newton's Law of Universal Gravitation states that every object with mass attracts every other object with mass, with a force that increases as the masses increase and decreases as the distance between the objects increases. The Law is described by the equation FG = G(M1M2/r2), where G is the gravitational constant, M1 and M2 are the masses of the objects, and r is the distance between them. While Newton's Law provided predictions of planetary orbits, it did not fully explain observations such as the precession of Mercury's orbit, problems addressed by Einstein's theory of general relativity.
Newtons Law of Universal Gravitation.ppt
Newton's Law of Universal Gravitation states that every object with mass attracts every other object with mass, with a force that increases as the masses increase and decreases as the distance between the objects increases. The Law is described by the equation FG = G(M1M2/r2), where G is the gravitational constant, M1 and M2 are the masses of the objects, and r is the distance between them. While Newton's Law provided predictions of planetary orbits, it did not fully explain observations such as the precession of Mercury's orbit, problems addressed by Einstein's theory of general relativity.
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Universal_Gravitation.ppt
Newton proposed 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. This law explained the force keeping the planets in orbit around the sun and the moon orbiting the Earth. Later experiments determined the proportionality constant in Newton's equation.
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1) Isaac Newton proposed a law of universal gravitation in 1666 stating that any two objects attract each other with a gravitational force proportional to the product of their masses and inversely proportional to the square of the distance between them.
2) The law explained the force keeping planets in orbit around the Sun and the Moon orbiting the Earth.
3) In 1798, Henry Cavendish experimentally determined the proportionality constant G in Newton's law of universal gravitation.
Universal gravitation arun
1) Isaac Newton formulated his law of universal gravitation in 1666, which states that any two objects attract each other with a force proportional to the product of their masses and inversely proportional to the square of the distance between them.
2) Henry Cavendish experimentally determined the proportionality constant G in 1798, which is equal to 6.67 x 10-11 N m2 / kg2.
3) Newton's law of universal gravitation explains why objects like the moon orbit the earth rather than falling straight down, and suggests that the force of gravity is universal across all masses in the universe.
Digital text
1) Gravitation is the fundamental force of attraction between objects with mass. Newton discovered that gravitation causes objects to be pulled toward each other, with a force that is directly proportional to their masses and inversely proportional to the square of the distance between them.
2) Newton formulated his universal law of gravitation after observing an apple fall from a tree and realizing that the same force must cause objects on Earth and celestial bodies like the moon to fall or orbit.
3) Newton's theory explained phenomena that were previously not understood, like why objects in orbit do not fly off into space, and it provided an understanding of gravity that lasted over two centuries until Einstein improved on the theory with his theory of general relativity.
Gravitation theory
1) Gravity is a natural phenomenon that causes all objects with mass to attract each other. Modern physics describes gravitation through Einstein's general theory of relativity, which views gravity as a distortion of spacetime by massive objects.
2) Isaac Newton formulated the law of universal gravitation, which 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) Newton's theory accounted for the motions of celestial bodies and dominated scientists' views of the physical universe for three centuries, until Einstein's general relativity resolved some discrepancies like Mercury's orbit.
Newtons Law of Universal Gravitation.ppt
Newton's Law of Universal Gravitation states that every object with mass attracts every other object with mass, with a force that increases as the masses increase and decreases as the distance between the objects increases. The Law is described by the equation FG = G(M1M2/r2), where G is the gravitational constant, M1 and M2 are the masses of the objects, and r is the distance between them. While Newton's Law provided predictions of planetary orbits, it did not fully explain observations such as the precession of Mercury's orbit, problems addressed by Einstein's theory of general relativity.
Newtons Law of Universal Gravitation.ppt
Newton's Law of Universal Gravitation states that every object with mass attracts every other object with mass, with a force that increases as the masses increase and decreases as the distance between the objects increases. The Law is described by the equation FG = G(M1M2/r2), where G is the gravitational constant, M1 and M2 are the masses of the objects, and r is the distance between them. While Newton's Law provided predictions of planetary orbits, it did not fully explain observations such as the precession of Mercury's orbit, problems addressed by Einstein's theory of general relativity.
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DOI: 10.13140/RG.2.2.25608.16648
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- Newton's law states that every point mass in the universe attracts every other point mass with a force directly proportional to the product of their masses and inversely proportional to the square of the distance between them.
- The law established that the gravitational force between any two objects depends on their masses and the distance between their centers, and explained many phenomena related to motion, such as why objects fall toward the ground and why planets orbit the sun.
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More from PaulAnicete2 (13)
PSE4_Lecture_Ch19- Heat & 1st Law of Thermodynamics.ppt
PSE4_Lecture_Ch19- Heat & 1st Law of Thermodynamics.ppt
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ESA/ACT Science Coffee: Diego Blas - Gravitational wave detection with orbita...
ESA/ACT Science Coffee: Diego Blas - Gravitational wave detection with orbita...Advanced-Concepts-Team
Presentation in the Science Coffee of the Advanced Concepts Team of the European Space Agency on the 07.06.2024.
Speaker: Diego Blas (IFAE/ICREA)
Title: Gravitational wave detection with orbital motion of Moon and artificial
Abstract:
In this talk I will describe some recent ideas to find gravitational waves from supermassive black holes or of primordial origin by studying their secular effect on the orbital motion of the Moon or satellites that are laser ranged.Direct Seeded Rice - Climate Smart Agriculture
Direct Seeded Rice - Climate Smart AgricultureInternational Food Policy Research Institute- South Asia Office
PPT on Direct Seeded Rice presented at the three-day 'Training and Validation Workshop on Modules of Climate Smart Agriculture (CSA) Technologies in South Asia' workshop on April 22, 2024.
Farming systems analysis: what have we learnt?.pptx
Presentation given at the official farewell of Prof Ken Gillet at Wageningen on 13 June 2024
ESR spectroscopy in liquid food and beverages.pptx
With increasing population, people need to rely on packaged food stuffs. Packaging of food materials requires the preservation of food. There are various methods for the treatment of food to preserve them and irradiation treatment of food is one of them. It is the most common and the most harmless method for the food preservation as it does not alter the necessary micronutrients of food materials. Although irradiated food doesn’t cause any harm to the human health but still the quality assessment of food is required to provide consumers with necessary information about the food. ESR spectroscopy is the most sophisticated way to investigate the quality of the food and the free radicals induced during the processing of the food. ESR spin trapping technique is useful for the detection of highly unstable radicals in the food. The antioxidant capability of liquid food and beverages in mainly performed by spin trapping technique.
(June 12, 2024) Webinar: Development of PET theranostics targeting the molecu...
(June 12, 2024) Webinar: Development of PET theranostics targeting the molecu...Scintica Instrumentation
Targeting Hsp90 and its pathogen Orthologs with Tethered Inhibitors as a Diagnostic and Therapeutic Strategy for cancer and infectious diseases with Dr. Timothy Haystead.The binding of cosmological structures by massless topological defects
Assuming spherical symmetry and weak field, it is shown that if one solves the Poisson equation or the Einstein field
equations sourced by a topological defect, i.e. a singularity of a very specific form, the result is a localized gravitational
field capable of driving flat rotation (i.e. Keplerian circular orbits at a constant speed for all radii) of test masses on a thin
spherical shell without any underlying mass. Moreover, a large-scale structure which exploits this solution by assembling
concentrically a number of such topological defects can establish a flat stellar or galactic rotation curve, and can also deflect
light in the same manner as an equipotential (isothermal) sphere. Thus, the need for dark matter or modified gravity theory is
mitigated, at least in part.
Compexometric titration/Chelatorphy titration/chelating titration
Classification
Metal ion ion indicators
Masking and demasking reagents
Estimation of Magnisium sulphate
Calcium gluconate
Complexometric Titration/ chelatometry titration/chelating titration, introduction, Types-
1.Direct Titration
2.Back Titration
3.Replacement Titration
4.Indirect Titration
Masking agent, Demasking agents
formation of complex
comparition between masking and demasking agents,
Indicators/Metal ion indicators/ Metallochromic indicators/pM indicators,
Visual Technique,PM indicators (metallochromic), Indicators of pH, Redox Indicators
Instrumental Techniques-Photometry
Potentiometry
Miscellaneous methods.
Complex titration with EDTA.
Gadgets for management of stored product pests_Dr.UPR.pdf
Insectsplayamajorroleinthedeteriorationoffoodgrainscausingbothquantitativeandqualitativelosses
Wellprovedthatnogranariescanbefilledwithgrainswithoutinsectsastheharvestedproducecontainegg(or)larvae(or)pupae(or)adultinsectinthembecauseoffieldcarryoverinfestationwhichcannotbeavoidedindevelopingcountrieslikeIndia
Simpletechnologiesfortimelydetectionofinsectsinthestoredproduceandtherebyplantimelycontrolmeasures
Applied Science: Thermodynamics, Laws & Methodology.pdf
When I was asked to give a companion lecture in support of ‘The Philosophy of Science’ (https://shorturl.at/4pUXz) I decided not to walk through the detail of the many methodologies in order of use. Instead, I chose to employ a long standing, and ongoing, scientific development as an exemplar. And so, I chose the ever evolving story of Thermodynamics as a scientific investigation at its best.
Conducted over a period of >200 years, Thermodynamics R&D, and application, benefitted from the highest levels of professionalism, collaboration, and technical thoroughness. New layers of application, methodology, and practice were made possible by the progressive advance of technology. In turn, this has seen measurement and modelling accuracy continually improved at a micro and macro level.
Perhaps most importantly, Thermodynamics rapidly became a primary tool in the advance of applied science/engineering/technology, spanning micro-tech, to aerospace and cosmology. I can think of no better a story to illustrate the breadth of scientific methodologies and applications at their best.
The cost of acquiring information by natural selection
This is a short talk that I gave at the Banff International Research Station workshop on Modeling and Theory in Population Biology. The idea is to try to understand how the burden of natural selection relates to the amount of information that selection puts into the genome.
It's based on the first part of this research paper:
The cost of information acquisition by natural selection
Ryan Seamus McGee, Olivia Kosterlitz, Artem Kaznatcheev, Benjamin Kerr, Carl T. Bergstrom
bioRxiv 2022.07.02.498577; doi: https://doi.org/10.1101/2022.07.02.498577
Micronuclei test.M.sc.zoology.fisheries.
Current Ms word generated power point presentation covers major details about the micronuclei test. It's significance and assays to conduct it. It is used to detect the micronuclei formation inside the cells of nearly every multicellular organism. It's formation takes place during chromosomal sepration at metaphase.
Randomised Optimisation Algorithms in DAPHNE
Slides from talk:
Aleš Zamuda: Randomised Optimisation Algorithms in DAPHNE .
Austrian-Slovenian HPC Meeting 2024 – ASHPC24, Seeblickhotel Grundlsee in Austria, 10–13 June 2024
https://ashpc.eu/
Travis Hills of MN is Making Clean Water Accessible to All Through High Flux ...
By harnessing the power of High Flux Vacuum Membrane Distillation, Travis Hills from MN envisions a future where clean and safe drinking water is accessible to all, regardless of geographical location or economic status.
Immersive Learning That Works: Research Grounding and Paths Forward
We will metaverse into the essence of immersive learning, into its three dimensions and conceptual models. This approach encompasses elements from teaching methodologies to social involvement, through organizational concerns and technologies. Challenging the perception of learning as knowledge transfer, we introduce a 'Uses, Practices & Strategies' model operationalized by the 'Immersive Learning Brain' and ‘Immersion Cube’ frameworks. This approach offers a comprehensive guide through the intricacies of immersive educational experiences and spotlighting research frontiers, along the immersion dimensions of system, narrative, and agency. Our discourse extends to stakeholders beyond the academic sphere, addressing the interests of technologists, instructional designers, and policymakers. We span various contexts, from formal education to organizational transformation to the new horizon of an AI-pervasive society. This keynote aims to unite the iLRN community in a collaborative journey towards a future where immersive learning research and practice coalesce, paving the way for innovative educational research and practice landscapes.
8.Isolation of pure cultures and preservation of cultures.pdf
Isolation of pure culture, its various method.
Recently uploaded (20)
ESA/ACT Science Coffee: Diego Blas - Gravitational wave detection with orbita...
ESA/ACT Science Coffee: Diego Blas - Gravitational wave detection with orbita...
Farming systems analysis: what have we learnt?.pptx
Farming systems analysis: what have we learnt?.pptx
GBSN - Biochemistry (Unit 6) Chemistry of Proteins
GBSN - Biochemistry (Unit 6) Chemistry of Proteins
ESR spectroscopy in liquid food and beverages.pptx
ESR spectroscopy in liquid food and beverages.pptx
(June 12, 2024) Webinar: Development of PET theranostics targeting the molecu...
(June 12, 2024) Webinar: Development of PET theranostics targeting the molecu...
The binding of cosmological structures by massless topological defects
The binding of cosmological structures by massless topological defects
Compexometric titration/Chelatorphy titration/chelating titration
Compexometric titration/Chelatorphy titration/chelating titration
aziz sancar nobel prize winner: from mardin to nobel
aziz sancar nobel prize winner: from mardin to nobel
Gadgets for management of stored product pests_Dr.UPR.pdf
Gadgets for management of stored product pests_Dr.UPR.pdf
Applied Science: Thermodynamics, Laws & Methodology.pdf
Applied Science: Thermodynamics, Laws & Methodology.pdf
The cost of acquiring information by natural selection
The cost of acquiring information by natural selection
Travis Hills of MN is Making Clean Water Accessible to All Through High Flux ...
Travis Hills of MN is Making Clean Water Accessible to All Through High Flux ...
Immersive Learning That Works: Research Grounding and Paths Forward
Immersive Learning That Works: Research Grounding and Paths Forward
8.Isolation of pure cultures and preservation of cultures.pdf
8.Isolation of pure cultures and preservation of cultures.pdf
PP16_-_Universal_Gravitation.ppt
- 1. Newton’s Law of Universal Gravitation Physics Mr. Berman
- 2. Isaac Newton 1666, England (45 years after Kepler).
- 3. Questions If the planets are orbiting the sun , what force is keeping them in orbit? What force keeps the moon in its orbit? Could the force of gravity be universal?
- 4. Newton’s Law of Universal Gravitation Any two objects attract each other with a gravitational force, proportional to the product of their masses and inversely proportional to the square of the distance between them. The force acts in the direction of the line connecting the centers of the masses.
- 5. Newton’s Law of Universal Gravitation http://scienceblogs.com/startswithabang/upload/2009/07/meet_our_second_moon/400px-NewtonsLawOfUniversalGravitation.svg.png
- 6. Why does the moon not fall straight down onto the earth?
- 8. The Value of G. G= 6.67 x 10-11 N m2 / kg2
- 9. Change of Gravitational Force with Distance Law of universal gravitation is known as an inverse square law.
- 10. Problem 1 Two spheres of mass 35kg are 60m apart. A) What force does one exert on the other? B) If the mass of one is tripled and the radius is quadrupled how does the force change?
- 11. Problem 2 Two spheres of equal mass have a force of gravity of 7x10-9 exerted on each other. If the distance between them is 7m, find the mass.
- 12. Problem 3 Find the value of the gravitational acceleration g. The mass of the earth is 6.0 x 1024kg.