Physicsjeopardy
•Download as PPT, PDF•
2 likes•399 views
The document contains questions and answers about concepts related to gravity, projectiles, and Newton's laws of motion. Some of the key points covered include: - Satellites need to be above the atmosphere to avoid air resistance. - The maximum projectile distance is achieved at a 45 degree angle. - Gravity accelerates objects at 9.8 m/s^2 near Earth's surface. - Newton's three laws of motion explain forces like inertia, acceleration, and action-reaction pairs between objects in contact.
Report
Share
Report
Share
Recommended
09
Friction is the force that opposes the relative motion or attempted motion of two surfaces in contact. Two examples of friction experienced daily are the friction between shoes and the ground when walking, and friction that allows brakes on vehicles to slow them down. Gravity is the force that attracts objects with mass towards one another, and its strength decreases with distance. On Earth, gravitational acceleration is approximately 9.8 m/s2.
Gravity and motion
Galileo showed that all objects accelerate at the same rate when falling, due to gravity, regardless of their mass. Heavier objects experience a greater force of gravity but require more force to accelerate them, so the acceleration is the same. Acceleration is the rate of change of an object's velocity over time and is directly proportional to the net force acting on an object and inversely proportional to its mass, as stated in Newton's Second Law of Motion. Newton's Three Laws of Motion describe the relationship between an object's motion and the forces acting upon it.
Ppt Gravity
The document discusses the law of universal gravitation and gravity. It states that all objects with mass exert gravitational attraction on each other, and that the gravitational force depends on the masses of the objects and the distance between them. It also explains that while the Earth exerts a force we can feel, we cannot feel the force of nearer objects like desks because their force is smaller due to lower mass and closer proximity.
Power Point Gravity
This document discusses gravity, weight, and weightlessness. It provides the formulas for calculating weight based on mass and gravitational acceleration. Your weight depends on the gravitational pull of the planet you are on. With no gravitational pull, you experience a state of weightlessness or neutral buoyancy. The document uses these concepts to calculate weight on different planets like Saturn based on their gravitational acceleration.
Gravity and motion class activity
The document discusses gravity and motion. It explains that all objects accelerate towards the Earth at 9.8 m/s due to gravity. Gravity is proportional to the product of the masses of objects and inversely proportional to the square of the distance between them. Newton's first law of motion states that objects at rest or in motion stay that way unless acted upon by an outside force, such as gravity.
Newton’s law of gravitation
Newton's law of universal gravitation 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 formula for this gravitational force is F = G(m1m2)/r^2, where F is the force of attraction, G is the gravitational constant, m1 and m2 are the masses of the two objects, and r is the distance between their centers of mass. The document provides examples of applying this formula to calculate gravitational forces between people, people and Earth, and people and objects.
6th Grade Chapter 10- forces and motion
Gravity is a force of attraction that acts between all objects with mass. Gravity causes all objects to accelerate towards each other at the same rate, so heavier and lighter objects fall at the same speed. The strength of gravity depends on the mass of the object, so gravity is stronger on large planets like Jupiter than on smaller bodies like the moon. Mass is a measure of the amount of matter in an object and does not change in different locations, while weight is the measure of the gravitational force acting on an object, so weight varies depending on the gravitational pull of different planets. Newton's three laws of motion describe how forces cause motion and changes in motion.
Newton's Laws & Gravitation
Newton's second law states that an object's acceleration depends on the net force acting on it and its mass. Force equals mass times acceleration. Newton's third law states that for every action there is an equal and opposite reaction. Gravity is a force between any two masses that depends on their masses and the distance between them, as described by the law of universal gravitation. In free fall, the only force acting is gravity, so all objects accelerate at the same rate due to gravity.
Recommended
09
Friction is the force that opposes the relative motion or attempted motion of two surfaces in contact. Two examples of friction experienced daily are the friction between shoes and the ground when walking, and friction that allows brakes on vehicles to slow them down. Gravity is the force that attracts objects with mass towards one another, and its strength decreases with distance. On Earth, gravitational acceleration is approximately 9.8 m/s2.
Gravity and motion
Galileo showed that all objects accelerate at the same rate when falling, due to gravity, regardless of their mass. Heavier objects experience a greater force of gravity but require more force to accelerate them, so the acceleration is the same. Acceleration is the rate of change of an object's velocity over time and is directly proportional to the net force acting on an object and inversely proportional to its mass, as stated in Newton's Second Law of Motion. Newton's Three Laws of Motion describe the relationship between an object's motion and the forces acting upon it.
Ppt Gravity
The document discusses the law of universal gravitation and gravity. It states that all objects with mass exert gravitational attraction on each other, and that the gravitational force depends on the masses of the objects and the distance between them. It also explains that while the Earth exerts a force we can feel, we cannot feel the force of nearer objects like desks because their force is smaller due to lower mass and closer proximity.
Power Point Gravity
This document discusses gravity, weight, and weightlessness. It provides the formulas for calculating weight based on mass and gravitational acceleration. Your weight depends on the gravitational pull of the planet you are on. With no gravitational pull, you experience a state of weightlessness or neutral buoyancy. The document uses these concepts to calculate weight on different planets like Saturn based on their gravitational acceleration.
Gravity and motion class activity
The document discusses gravity and motion. It explains that all objects accelerate towards the Earth at 9.8 m/s due to gravity. Gravity is proportional to the product of the masses of objects and inversely proportional to the square of the distance between them. Newton's first law of motion states that objects at rest or in motion stay that way unless acted upon by an outside force, such as gravity.
Newton’s law of gravitation
Newton's law of universal gravitation 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 formula for this gravitational force is F = G(m1m2)/r^2, where F is the force of attraction, G is the gravitational constant, m1 and m2 are the masses of the two objects, and r is the distance between their centers of mass. The document provides examples of applying this formula to calculate gravitational forces between people, people and Earth, and people and objects.
6th Grade Chapter 10- forces and motion
Gravity is a force of attraction that acts between all objects with mass. Gravity causes all objects to accelerate towards each other at the same rate, so heavier and lighter objects fall at the same speed. The strength of gravity depends on the mass of the object, so gravity is stronger on large planets like Jupiter than on smaller bodies like the moon. Mass is a measure of the amount of matter in an object and does not change in different locations, while weight is the measure of the gravitational force acting on an object, so weight varies depending on the gravitational pull of different planets. Newton's three laws of motion describe how forces cause motion and changes in motion.
Newton's Laws & Gravitation
Newton's second law states that an object's acceleration depends on the net force acting on it and its mass. Force equals mass times acceleration. Newton's third law states that for every action there is an equal and opposite reaction. Gravity is a force between any two masses that depends on their masses and the distance between them, as described by the law of universal gravitation. In free fall, the only force acting is gravity, so all objects accelerate at the same rate due to gravity.
LO1-Force
The document defines key concepts related to force, including that a Newton is the unit of force equal to the force needed to accelerate 1 kg mass by 1 m/s^2. It also defines mass as a measure of inertia, and weight as the force of gravity acting on a body. An example calculation is provided where the force on a 5 kg object dropped and hitting the ground is calculated as 49 Newtons using the formula Force = Mass x Acceleration.
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.
Newton's Three Laws of Motion
Newton's Laws describe the motion of objects. Newton's First Law states that objects at rest stay at rest and objects in motion stay in motion with the same speed and direction unless acted upon by an unbalanced force. Newton's Second Law states that the acceleration of an object as produced by a net force is directly proportional to the magnitude of the net force, and inversely proportional to the object's mass. Newton's Third Law states that for every action, there is an equal and opposite reaction. Free-body diagrams are used to identify all the forces acting on an object and indicate the directions of the forces.
Rockets internet.ppt
The document discusses Newton's second and third laws of motion and how they relate to rocket propulsion. It explains that rockets accelerate due to unbalanced forces from the ejection of exhaust particles, as per Newton's third law of action and reaction. Different rocket designs eject particles of varying mass, affecting their thrust according to the formula force equals mass times acceleration. The document provides examples of water rockets, balloon rockets, and real rockets to illustrate how thrust can be varied based on the mass and speed of exhaust particles.
Rajat manchanda
The document discusses Newton's three laws of motion:
1) An object at rest stays at rest and an object in motion stays in motion unless acted upon by an unbalanced force. Friction causes moving objects to slow down.
2) The acceleration of an object as produced by a net force is directly proportional to the magnitude of the net force, in the same direction as the net force, and inversely proportional to the mass of the object.
3) For every action, there is an equal and opposite reaction. The forces acting between two interacting objects are equal in magnitude but opposite in direction.
Gravity
The document discusses gravity from both a scientific and Islamic perspective. It defines gravity as a natural force that attracts objects with mass towards each other. It explains how gravity allows life to exist on Earth by giving objects weight and settling them on the planet's surface. The Quran references gravity through verses describing Allah making Earth a stable home. Overall, the document aims to demonstrate science and religion are compatible by showing the Quran discussed gravity centuries before its scientific discovery.
Anti gravity
The document discusses anti-gravity, which refers to creating objects free from the force of gravity. It notes that while anti-gravity is common in science fiction, general relativity suggests it is impossible except under contrived circumstances. One proposed method for producing anti-gravity involves using negative mass, where a negative mass object would fall towards normal matter due to repulsive gravitational forces.
Gravity for kids
Gravity is the force that attracts objects to each other. Galileo proved that all objects fall at the same rate regardless of mass. Isaac Newton furthered understanding by describing gravity mathematically as a force dependent on the masses of objects and the distance between them. Newton's law of universal gravitation explained phenomena like planetary orbits and the moon's effect in causing ocean tides through its gravitational pull on Earth.
Gravity mass weight
Gravity is an invisible force that pulls objects with mass towards the center of planets like Earth. Gravity gives objects weight, which is measured in Newtons and describes the force of gravitational pull, while mass describes the amount of material in an object and does not change in different gravitational fields. On Earth, a 50kg person has a weight of 500 Newtons, but their mass would remain 50kg on the Moon where gravity is weaker - there their weight would be 83.3 Newtons due to the lower gravitational pull.
Gravity lesson
1) Gravity is an attractive force that pulls objects towards the center of massive bodies like the Earth.
2) Sir Isaac Newton discovered gravity through his observations of apples falling from trees and was able to mathematically explain gravity.
3) The strength of gravity varies on different planets, with larger planets like Jupiter having stronger gravitational pull than smaller planets like Pluto.
Newton’s universal law of gravitation
Sir Isaac Newton discovered gravity and formulated the law of universal gravitation by observing an apple fall from a tree in the late 1600s. Newton's law states that every object in the universe attracts every other object with a force that is directly proportional to the product of their masses and inversely proportional to the square of the distance between them. The law of universal gravitation explains that all objects experience an attractive gravitational force towards one another, with the force being stronger between objects with greater mass and weaker over greater distances.
Forces & Changes in Motion
The document compares the world record breaking skydives of Joe Kittinger in 1960 and Felix Baumgartner in 2012, noting that Baumgartner jumped from a higher altitude of 39,045m compared to Kittinger's 31,300m, allowing Baumgartner to reach a higher maximum speed of 1342.8 km/h over Kittinger's 988km/h. The document also explores the factors like air pressure and density that influence terminal velocity and made Baumgartner's higher jump necessary to break the speed of sound record.
Gravity and laws of motion power point2
This document summarizes Sir Isaac Newton's three Laws of Motion and the Law of Universal Gravitation. It explains that the first law states that an object at rest stays at rest and an object in motion stays in motion unless acted upon by an outside force. The second law states that the acceleration of an object depends on its mass and the applied force. The third law states that for every action there is an equal and opposite reaction. It also describes gravity as the force that attracts objects toward Earth's center and explains how gravitational attraction depends on mass and distance between objects.
Newton's law of motion
Newton's laws of motion are three physical laws that, together, laid the foundation for classical mechanics. They describe the relationship between a body and the forces acting upon it, and its motion in response to those forces.
Newton's law
- Aristotle believed that objects have a natural place and will return to that place after being moved by force. Isaac Newton later proposed that objects tend to stay in their current state of motion unless acted on by an unbalanced force.
- Newton published his three laws of motion in 1687, including the first law that an object at rest or in motion stays at rest or in motion unless acted on by an outside force.
- Forces can be contact forces that require touching an object or long-range forces like gravity that act over a distance. Forces have agents that are the direct cause of the force.
Gravity And Motion
Galileo Galilei demonstrated through dropping objects of different masses from the Leaning Tower of Pisa that all objects accelerate at the same rate when falling, disregarding air resistance. While heavier objects experience a greater gravitational force, they also have more mass and are thus equally difficult to accelerate. As a result, the acceleration due to gravity is the same for all objects and can be used to calculate change in velocity over time for falling objects. However, air resistance also affects the motion of falling objects depending on their size, shape, and speed.
Giancoli - Chapter 5 - Section 5.6 - 5.9 - Universal Gravitation
Slides that go with Giancoli Chapter 5 section 5.6 to 5.9 on Universal Gravitation, Satellites, Weightlessness, and Kepler's Laws.
Notes 3.3
Newton's 3rd law states that for every action, there is an equal and opposite reaction. Momentum is the product of an object's mass and velocity. The law of conservation of momentum states that the total momentum of a system remains constant if no external forces act on it. An example calculation shows how to determine the velocity of a ball thrown in the opposite direction of a moving skateboarder using the law of conservation of momentum.
"Force and motion" is a power point for the 9th grade Physics students at the...
1) A force is any push or pull that causes an object to change its motion or shape. Forces come in pairs - whenever one object exerts a force on another, the second object exerts an equal and opposite force back.
2) Newton's Second Law states that the acceleration of an object is directly proportional to the net force acting on it, and inversely proportional to its mass. Acceleration and net force always point in the same direction.
3) Newton's First Law says that objects at rest stay at rest and objects in motion stay in motion with the same speed and direction unless acted upon by a net unbalanced force.
Notes 3.1
1. Sir Isaac Newton formulated the basic laws of mechanics in the late 1600s, including Newton's Three Laws of Motion.
2. Newton's First Law states that an object at rest stays at rest and an object in motion stays in motion with the same speed and in the same direction unless acted upon by an unbalanced force.
3. Newton's Second Law states that the acceleration of an object as produced by a net force is directly proportional to the magnitude of the net force, in the same direction as the net force, and inversely proportional to the mass of the object.
Heywire Winners Announcement, Canberra 2007
This was the audio visual presentation for the announcement of the 2007 ABC Radio Heywire winners, at the Riverhealth Conference in Canberra.
Beijing to Burketown by Jane Hardy
n our first in a series of features from former Heywire Alumni, Heywire 2000 winner Jane Hardy has put together an incredible multimedia experience comparing the similarities between Beijing, a city of almost 16 million people and Burketown, a city of 160 people.
To read the web feature visit:
http://blogs.abc.net.au/heywire/2008/01/beijing-to-burk.html
More Related Content
What's hot
LO1-Force
The document defines key concepts related to force, including that a Newton is the unit of force equal to the force needed to accelerate 1 kg mass by 1 m/s^2. It also defines mass as a measure of inertia, and weight as the force of gravity acting on a body. An example calculation is provided where the force on a 5 kg object dropped and hitting the ground is calculated as 49 Newtons using the formula Force = Mass x Acceleration.
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.
Newton's Three Laws of Motion
Newton's Laws describe the motion of objects. Newton's First Law states that objects at rest stay at rest and objects in motion stay in motion with the same speed and direction unless acted upon by an unbalanced force. Newton's Second Law states that the acceleration of an object as produced by a net force is directly proportional to the magnitude of the net force, and inversely proportional to the object's mass. Newton's Third Law states that for every action, there is an equal and opposite reaction. Free-body diagrams are used to identify all the forces acting on an object and indicate the directions of the forces.
Rockets internet.ppt
The document discusses Newton's second and third laws of motion and how they relate to rocket propulsion. It explains that rockets accelerate due to unbalanced forces from the ejection of exhaust particles, as per Newton's third law of action and reaction. Different rocket designs eject particles of varying mass, affecting their thrust according to the formula force equals mass times acceleration. The document provides examples of water rockets, balloon rockets, and real rockets to illustrate how thrust can be varied based on the mass and speed of exhaust particles.
Rajat manchanda
The document discusses Newton's three laws of motion:
1) An object at rest stays at rest and an object in motion stays in motion unless acted upon by an unbalanced force. Friction causes moving objects to slow down.
2) The acceleration of an object as produced by a net force is directly proportional to the magnitude of the net force, in the same direction as the net force, and inversely proportional to the mass of the object.
3) For every action, there is an equal and opposite reaction. The forces acting between two interacting objects are equal in magnitude but opposite in direction.
Gravity
The document discusses gravity from both a scientific and Islamic perspective. It defines gravity as a natural force that attracts objects with mass towards each other. It explains how gravity allows life to exist on Earth by giving objects weight and settling them on the planet's surface. The Quran references gravity through verses describing Allah making Earth a stable home. Overall, the document aims to demonstrate science and religion are compatible by showing the Quran discussed gravity centuries before its scientific discovery.
Anti gravity
The document discusses anti-gravity, which refers to creating objects free from the force of gravity. It notes that while anti-gravity is common in science fiction, general relativity suggests it is impossible except under contrived circumstances. One proposed method for producing anti-gravity involves using negative mass, where a negative mass object would fall towards normal matter due to repulsive gravitational forces.
Gravity for kids
Gravity is the force that attracts objects to each other. Galileo proved that all objects fall at the same rate regardless of mass. Isaac Newton furthered understanding by describing gravity mathematically as a force dependent on the masses of objects and the distance between them. Newton's law of universal gravitation explained phenomena like planetary orbits and the moon's effect in causing ocean tides through its gravitational pull on Earth.
Gravity mass weight
Gravity is an invisible force that pulls objects with mass towards the center of planets like Earth. Gravity gives objects weight, which is measured in Newtons and describes the force of gravitational pull, while mass describes the amount of material in an object and does not change in different gravitational fields. On Earth, a 50kg person has a weight of 500 Newtons, but their mass would remain 50kg on the Moon where gravity is weaker - there their weight would be 83.3 Newtons due to the lower gravitational pull.
Gravity lesson
1) Gravity is an attractive force that pulls objects towards the center of massive bodies like the Earth.
2) Sir Isaac Newton discovered gravity through his observations of apples falling from trees and was able to mathematically explain gravity.
3) The strength of gravity varies on different planets, with larger planets like Jupiter having stronger gravitational pull than smaller planets like Pluto.
Newton’s universal law of gravitation
Sir Isaac Newton discovered gravity and formulated the law of universal gravitation by observing an apple fall from a tree in the late 1600s. Newton's law states that every object in the universe attracts every other object with a force that is directly proportional to the product of their masses and inversely proportional to the square of the distance between them. The law of universal gravitation explains that all objects experience an attractive gravitational force towards one another, with the force being stronger between objects with greater mass and weaker over greater distances.
Forces & Changes in Motion
The document compares the world record breaking skydives of Joe Kittinger in 1960 and Felix Baumgartner in 2012, noting that Baumgartner jumped from a higher altitude of 39,045m compared to Kittinger's 31,300m, allowing Baumgartner to reach a higher maximum speed of 1342.8 km/h over Kittinger's 988km/h. The document also explores the factors like air pressure and density that influence terminal velocity and made Baumgartner's higher jump necessary to break the speed of sound record.
Gravity and laws of motion power point2
This document summarizes Sir Isaac Newton's three Laws of Motion and the Law of Universal Gravitation. It explains that the first law states that an object at rest stays at rest and an object in motion stays in motion unless acted upon by an outside force. The second law states that the acceleration of an object depends on its mass and the applied force. The third law states that for every action there is an equal and opposite reaction. It also describes gravity as the force that attracts objects toward Earth's center and explains how gravitational attraction depends on mass and distance between objects.
Newton's law of motion
Newton's laws of motion are three physical laws that, together, laid the foundation for classical mechanics. They describe the relationship between a body and the forces acting upon it, and its motion in response to those forces.
Newton's law
- Aristotle believed that objects have a natural place and will return to that place after being moved by force. Isaac Newton later proposed that objects tend to stay in their current state of motion unless acted on by an unbalanced force.
- Newton published his three laws of motion in 1687, including the first law that an object at rest or in motion stays at rest or in motion unless acted on by an outside force.
- Forces can be contact forces that require touching an object or long-range forces like gravity that act over a distance. Forces have agents that are the direct cause of the force.
Gravity And Motion
Galileo Galilei demonstrated through dropping objects of different masses from the Leaning Tower of Pisa that all objects accelerate at the same rate when falling, disregarding air resistance. While heavier objects experience a greater gravitational force, they also have more mass and are thus equally difficult to accelerate. As a result, the acceleration due to gravity is the same for all objects and can be used to calculate change in velocity over time for falling objects. However, air resistance also affects the motion of falling objects depending on their size, shape, and speed.
Giancoli - Chapter 5 - Section 5.6 - 5.9 - Universal Gravitation
Slides that go with Giancoli Chapter 5 section 5.6 to 5.9 on Universal Gravitation, Satellites, Weightlessness, and Kepler's Laws.
Notes 3.3
Newton's 3rd law states that for every action, there is an equal and opposite reaction. Momentum is the product of an object's mass and velocity. The law of conservation of momentum states that the total momentum of a system remains constant if no external forces act on it. An example calculation shows how to determine the velocity of a ball thrown in the opposite direction of a moving skateboarder using the law of conservation of momentum.
"Force and motion" is a power point for the 9th grade Physics students at the...
1) A force is any push or pull that causes an object to change its motion or shape. Forces come in pairs - whenever one object exerts a force on another, the second object exerts an equal and opposite force back.
2) Newton's Second Law states that the acceleration of an object is directly proportional to the net force acting on it, and inversely proportional to its mass. Acceleration and net force always point in the same direction.
3) Newton's First Law says that objects at rest stay at rest and objects in motion stay in motion with the same speed and direction unless acted upon by a net unbalanced force.
Notes 3.1
1. Sir Isaac Newton formulated the basic laws of mechanics in the late 1600s, including Newton's Three Laws of Motion.
2. Newton's First Law states that an object at rest stays at rest and an object in motion stays in motion with the same speed and in the same direction unless acted upon by an unbalanced force.
3. Newton's Second Law states that the acceleration of an object as produced by a net force is directly proportional to the magnitude of the net force, in the same direction as the net force, and inversely proportional to the mass of the object.
What's hot (20)
Giancoli - Chapter 5 - Section 5.6 - 5.9 - Universal Gravitation
Giancoli - Chapter 5 - Section 5.6 - 5.9 - Universal Gravitation
"Force and motion" is a power point for the 9th grade Physics students at the...
"Force and motion" is a power point for the 9th grade Physics students at the...
Viewers also liked
Heywire Winners Announcement, Canberra 2007
This was the audio visual presentation for the announcement of the 2007 ABC Radio Heywire winners, at the Riverhealth Conference in Canberra.
Beijing to Burketown by Jane Hardy
n our first in a series of features from former Heywire Alumni, Heywire 2000 winner Jane Hardy has put together an incredible multimedia experience comparing the similarities between Beijing, a city of almost 16 million people and Burketown, a city of 160 people.
To read the web feature visit:
http://blogs.abc.net.au/heywire/2008/01/beijing-to-burk.html
Newton’S Laws Practice
1) The document contains 30 multiple choice questions about Newton's Laws of motion, forces, and related concepts like mass, weight, and inertia.
2) Many questions focus on identifying examples that demonstrate Newton's First Law of inertia and Third Law of equal and opposite forces.
3) Other questions ask about calculating acceleration given force and mass or vice versa, as well as identifying which object has more mass in different gravitational contexts.
PRESENTATION ABOUT SYN - ABAF
This is a presentation that I gave to the Australian Business Arts Foundation, introducing and explaining the concept of SYN (The Student Youth Network) in Melbourne.
Mlearn 2011 conference keynote
This document discusses a study that compared the effectiveness of different modes of mobile interaction for learning English vocabulary among Japanese high school students. The study found no significant differences in learning outcomes between using an adaptive e-book app, a regular e-book reader, or a paper book. Challenges included the books being too difficult, lack of student motivation or free time, and technology that was not engaging. However, international collaboration on mobile learning continues with the goal of designing more effective adaptive learning technologies to bridge cultural and educational divides globally.
Running a Gaming Program When You Can't Tell the Difference Between an Xbox a...
Presentation given at Internet Librarian 2007 conference by Josh Weiland, Webmaster & Unofficial Gaming Guru, and Maryann Mori, Teen Specialist Librarian & Supervisor of Popular Materials Center, both employees of the Evansville Vanderburgh Public Library system.
Bibliography available online at http://www.evpl.org/gaming.
Sioux Hot-or-Not: The future of Linux (Alan Cox)
Alan Cox discusses how various technological and business trends will influence the future development of Linux. Hardware is evolving towards multi-core processors and more dynamic configuration. Software priorities are changing due to demands for security, power management, and real-time performance. Legal issues and business needs will also impact Linux's continued evolution.
Alumni Presentation - Homecoming 2007
This document outlines plans to improve the alumni experience for the Tau Delta chapter of AEPi. It discusses establishing an alumni advisory board and foundation to facilitate mentorship, fundraising and chapter support. A survey of alumni found that they want more involvement opportunities, chapter updates and networking with other alumni. The chapter will enhance communications through an improved quarterly newsletter, online updates and a dedicated alumni website. They will also expand alumni programming at homecoming and other events both in the Chicago area and elsewhere.
Rollbase Mobile Tech Tips
The document provides tips for using Progress Rollbase Mobile to build mobile apps faster. It outlines three tech tips presented in videos that show how to enable existing Rollbase objects and services for mobile, build a mobile UI by binding to Rollbase objects and views, and add push notifications. The document encourages trying Progress Rollbase Mobile to enhance the app building experience.
Beijing to Burketown by Jane Hardy
In our first in a series of features from former Heywire Alumni, Heywire 2000 winner Jane Hardy has put together an incredible multimedia experience comparing the similarities between Beijing, a city of almost 16 million people and Burketown, a city of 160 people.
Ingl Sfacillight
This document contains a collection of Spanish phrases and idioms. Many of the phrases are nonsensical or humorous when taken out of context. Some examples include "You have more tale than little street", "Your pan has gone", and "Coward of the prairie". The phrases reference various topics but do not form a coherent story or provide much meaningful information on their own.
Mobile Phone To Computer
The document discusses emerging trends in mobile technology and usage. It covers 3 main topics: 1) The human-machine interface is becoming more sophisticated with interfaces that go beyond menus and forms to command line controls for apps. 2) Hardware trends include more open platforms and improvements in areas like mesh networks and power. 3) Understanding user ethnographics is important, as revealed in studies showing preferences for shared/cheap phones and basic needs over high-end features. Simple, low-cost phones still have value even in developed markets.
Lewis Diagram
The document discusses Lewis diagrams and the octet rule for drawing molecular structures. It notes that most atoms form bonds to gain eight valence electrons, with exceptions for hydrogen, groups 1-3, and atoms that can exceed eight electrons. It provides instructions for drawing Lewis diagrams: determine total valence electrons, arrange atoms with singular in middle, form bonds between atoms, and distribute remaining electrons to give each atom an octet where possible. Examples of drawing Lewis diagrams for CF4, BeCl2, and CO2 are included to demonstrate the process.
Reference Scope Identification in Citing Sentences
This document describes an approach to identify the scope of references in sentences containing multiple citations. The approach uses a conditional random field (CRF) sequence model with features including distance, position, part-of-speech tags, and syntactic dependencies. It first segments sentences using punctuation and conjunctions, then applies the CRF and a majority voting scheme to label each word as inside or outside the scope. The method achieved over 90% accuracy on a dataset of citations from ACL papers.
Facultys fear openness - EduHub Days 2011
The document discusses the faculty's fear of openness in education. It outlines 5 common fears: 1) openness may damage reputation if poor materials are shared, 2) may impede teaching if students see materials in another class, 3) may endanger careers if open publishing replaces traditional publishing, 4) may lead to legal issues around copyright, and 5) may result in financial losses if materials can be freely downloaded instead of buying textbooks. The document asks how to respond to these objections to openness in education.
Viewers also liked (20)
Running a Gaming Program When You Can't Tell the Difference Between an Xbox a...
Running a Gaming Program When You Can't Tell the Difference Between an Xbox a...
Reference Scope Identification in Citing Sentences
Reference Scope Identification in Citing Sentences
Similar to Physicsjeopardy
Newtons law of motion grade 8
Sir Isaac Newton was an English physicist and mathematician born in 1642 who made seminal contributions to the fields of natural philosophy, mathematics, astronomy, and optics. He is most famous for formulating the three laws of motion, including:
1) An object at rest stays at rest and an object in motion stays in motion with the same speed and in the same direction unless acted upon by an unbalanced force.
2) The acceleration of an object as produced by a net force is directly proportional to the magnitude of the net force, in the same direction as the net force, and inversely proportional to the mass of the object.
3) For every action, there is an equal and opposite reaction.
newtonslawofmotion-140725083419-phpapp02.pdf
Sir Isaac Newton was an English physicist and mathematician born in 1642 who made seminal contributions to the fields of natural philosophy, mathematics, astronomy, and optics. He is most famous for formulating the three laws of motion:
1) An object at rest stays at rest and an object in motion stays in motion with the same speed and in the same direction unless acted upon by an unbalanced force.
2) The acceleration of an object as produced by a net force is directly proportional to the magnitude of the net force, in the same direction as the net force, and inversely proportional to the mass of the object.
3) For every action, there is an equal and opposite reaction.
Newton
Rajat manchanda
The document discusses Newton's three laws of motion:
1) An object at rest stays at rest and an object in motion stays in motion unless acted upon by an unbalanced force. Friction causes moving objects to slow down.
2) The acceleration of an object as produced by a net force is directly proportional to the magnitude of the net force, in the same direction as the net force, and inversely proportional to the mass of the object.
3) For every action, there is an equal and opposite reaction. The forces acting between two interacting objects are equal in magnitude but opposite in direction.
Newtons Laws Of Motion
Newton's three laws of motion are summarized as follows:
1) An object at rest stays at rest and an object in motion stays in motion with the same speed and in the same direction unless acted upon by an unbalanced force.
2) The acceleration of an object as produced by a force is directly proportional to the force magnitude and inversely proportional to the mass of the object.
3) For every action, there is an equal and opposite reaction.
Lesson 2 Motion and Conservation Laws.ppt
This document provides an overview of motion and conservation laws. It begins by explaining Aristotle's conception of motion as natural or violent, then Galileo's rejection of the idea that a force is needed to maintain motion. It then covers Newton's three laws of motion and uses them to explain why objects fall at the same rate regardless of mass. The document also discusses conservation of mass, energy, and momentum. It provides examples of applying the laws of conservation to collisions and gravitational interactions.
Forces
The document discusses different types of forces including gravitational, electromagnetic, weak nuclear, and strong nuclear forces. It also covers Newton's three laws of motion, defining inertia, mass, weight, net force, and friction. Key concepts are that mass is a measure of an object's quantity of matter independent of gravity, while weight depends on gravity. Newton's second law states that force equals mass times acceleration, and his third law is that for every action there is an equal and opposite reaction. Friction opposes motion between surfaces in contact.
Forces
Forces can cause objects to move, change speed or direction, turn, bend or twist. Forces can be contact forces that act through direct physical contact, like pushing or pulling, or non-contact forces that act over a distance, like magnetism or gravity. Balanced forces cause no change in motion, while unbalanced forces cause acceleration or changes in speed or direction. Newton's three laws of motion describe how forces affect the motion of objects.
Newtons laws of motion
This document discusses Newton's three laws of motion:
1) Law of Inertia - An object at rest stays at rest and an object in motion stays in motion unless acted upon by an unbalanced force.
2) Second Law - Force equals mass times acceleration (F=ma).
3) Third Law - For every action there is an equal and opposite reaction. Examples are provided for each law, such as friction causing objects to slow down due to the first law, and calculations using the second law equation.
2nd Law.ppt
This document discusses Newton's second law of motion. It states that the acceleration of an object is directly proportional to the net force acting on it and inversely proportional to its mass. Newton's second law is expressed by the equation F=ma, where F is the net force, m is the mass of the object, and a is the acceleration. Several examples are provided to illustrate Newton's second law in everyday situations like pushing cars or trucks with the same force. Newton's third law of motion, which states that for every action there is an equal and opposite reaction, is also discussed along with examples.
Lecture 3 newton_laws
1) Newton's three laws of motion are described, including the first law of inertia, the second law relating force, mass and acceleration, and the third law of equal and opposite reactions.
2) The first law states that an object at rest stays at rest and an object in motion stays in motion unless acted on by an unbalanced force. Friction is given as an example of a force that can slow objects down.
3) The second law establishes the formula F=ma, where force equals mass times acceleration. Several examples are given to illustrate applications of this law.
Newton's laws of motion
This document summarizes Newton's three laws of motion:
1) An object at rest stays at rest and an object in motion stays in motion unless acted upon by an unbalanced force. This law is known as the law of inertia.
2) The acceleration of an object as produced by a net force is directly proportional to the magnitude of the net force, in the same direction as the net force, and inversely proportional to the mass of the object. This is expressed by F=ma.
3) For every action, there is an equal and opposite reaction. The forces of action and reaction between two objects always act in opposite directions.
Newtons laws of_motion
A powerpoint i used for a STEM Presetation on using Dukane products with STEM( Science , Technology, Engineering and Math).
Bill McIntosh
SchoolVision Inc ( my consulting company)
Authorized Dukane/Convey Consultant
Phone :843-442-8888
Email :WKMcIntosh@Comcast.net
Twitter : @OtisTMcIntosh
SchoolVision Website on Facebook: https://www.facebook.com/WKMIII
newtons_laws_of_motion.ppt
This document provides information about Newton's Three Laws of Motion:
1) Newton's First Law of Motion (Law of Inertia) states that an object at rest stays at rest and an object in motion stays in motion with the same speed and in the same direction unless acted upon by an unbalanced force. Friction is given as an example of a force that can cause an object in motion to slow down and stop.
2) Newton's Second Law of Motion (Law of Acceleration) states that the net force on an object equals its mass times its acceleration (F=ma). Examples are given to demonstrate how acceleration depends on mass and net force.
3) Newton's Third Law of Motion
Newtons Laws Of Motion
Newton's three laws of motion are summarized as follows:
1) An object at rest stays at rest and an object in motion stays in motion unless acted upon by an unbalanced force (law of inertia).
2) The acceleration of an object as produced by a net force is directly proportional to the magnitude of the net force, in the same direction as the net force, and inversely proportional to the mass of the object (F=ma).
3) For every action, there is an equal and opposite reaction.
Newtons laws of_motion
Newton's three laws of motion are summarized as follows:
1) An object at rest stays at rest and an object in motion stays in motion unless acted upon by an unbalanced force (law of inertia).
2) The acceleration of an object as produced by a net force is directly proportional to the magnitude of the net force, in the same direction as the net force, and inversely proportional to the mass of the object (F=ma).
3) For every action, there is an equal and opposite reaction.
Bs ed,gen sc,unit # 10,11,12,laws of motion.
Newton's three laws of motion are summarized. Newton's First Law states that objects at rest stay at rest and objects in motion stay in motion unless acted upon by an unbalanced force. Newton's Second Law states that force equals mass times acceleration. Newton's Third Law states that for every action, there is an equal and opposite reaction. Examples are provided to illustrate each law, such as friction slowing moving objects or gravity accelerating objects at the same rate but with different forces depending on their mass.
Introduction to friction
This document discusses Newton's three laws of motion:
1) An object at rest stays at rest and an object in motion stays in motion unless acted upon by an unbalanced force.
2) The acceleration of an object as produced by a net force is directly proportional to the magnitude of the net force, in the same direction as the net force, and inversely proportional to the mass of the object.
3) For every action, there is an equal and opposite reaction. The document provides several examples to illustrate each law, such as friction slowing objects in motion, forces needed to accelerate objects of different masses, and action-reaction force pairs in phenomena like flight.
Newtons laws of_motion
1) Newton's laws of motion describe the relationship between an object and the forces acting upon it. The three laws are: Law of Inertia, F=ma, and Action-Reaction.
2) The Law of Inertia states that an object at rest stays at rest and an object in motion stays in motion unless acted upon by an unbalanced force.
3) Newton's Second Law, F=ma, defines the relationship between the net force (F), mass (m), and acceleration (a) of an object.
Newtons Laws Of Motion 2
The document discusses Newton's three laws of motion:
1) An object at rest stays at rest and an object in motion stays in motion unless acted upon by an unbalanced force.
2) The acceleration of an object as produced by a net force is directly proportional to the magnitude of the net force, in the same direction as the net force, and inversely proportional to the mass of the object.
3) For every action, there is an equal and opposite reaction.
Newton
The document discusses Newton's three laws of motion:
1) An object at rest stays at rest and an object in motion stays in motion unless acted upon by an unbalanced force.
2) The acceleration of an object as produced by a net force is directly proportional to the magnitude of the net force, in the same direction as the net force, and inversely proportional to the mass of the object.
3) For every action, there is an equal and opposite reaction.
Similar to Physicsjeopardy (20)
More from kitcoffeen
Chembond
Chemical bonds form between atoms in different ways depending on electron configuration. Ionic bonds form when electrons are transferred between metals and nonmetals, creating positively and negatively charged ions. Covalent bonds form when electrons are shared between nonmetals. Metallic bonds form between metal atoms through a "sea of electrons" that holds the atoms together.
Chembond
Chemical bonds form between atoms in order to fill their outer electron shells. Ionic bonds form when electrons are transferred between metals and nonmetals, creating positively and negatively charged ions. Covalent bonds form when electrons are shared between nonmetals. Metallic bonds form between metal atoms through a "sea of electrons".
Review Week2
Vectors can represent both direction and magnitude, while scalars represent only magnitude. Acceleration can be negative. When vectors are going in the same direction, you add them together, and when they are going in opposite directions, you subtract them. If an object moves and returns to its original position, its distance vector is zero. Mass stays the same in different gravitational fields, while weight can change. Weight is the measurement of gravitational force on an object. Acceleration due to gravity is approximately 9.8 m/s^2. Heavier objects do not fall faster than lighter objects because gravity accelerates all objects at the same rate regardless of mass. Terminal velocity is reached when air resistance equals the downward pull of gravity.
Phyrev3
A distant planet has 3 times the gravitational force of Earth, so a 100g object would have a mass of 300g there. A boat is propelled forward by a sail exerting 5N of force and an engine exerting 20N of force, so the net forward force on the boat is 25N. A waiter adds water to a glass before performing a trick of pulling a tablecloth out from under objects to prevent the glass from breaking when it would have no liquid in it.
Phyrev4
The document contains review questions about momentum, impulse, and the conservation of momentum. It asks about the equations for momentum and impulse, examples of their application like a bird's momentum and a truck's runaway ramp, and problems involving conservation of momentum such as a fish swallowing another fish or a person jumping out of a moving golf cart. It also questions the differences between elastic and inelastic collisions, and how impulse relates to safely catching or stopping moving objects without damage.
Chemrev4
This document contains review questions covering topics in waves, emission and the Bohr model, electrons, and photon properties. It asks about wavelength, Planck's constant, the speed of light, electron configurations for various elements, filling electron orbitals according to Aufbau principle, converting between units of length and frequency, and using formulas relating energy, Planck's constant, frequency, and wavelength of electromagnetic waves including photons.
Chemrev5
The periodic law states that the physical and chemical properties of elements are periodic functions of their atomic numbers. Dmitri Mendeleev was the first to organize the elements into the periodic table based on their atomic masses. Glenn Seaborg later refined the periodic table by arranging the elements according to their atomic numbers.
Chem Rev3
The document provides information about average atomic mass calculations for vanadium isotopes, molar conversions for osmium, lead, and technetium, and the number of copper atoms in a 200g copper nugget. It also includes questions about converting between moles and grams of magnesium and properties of waves, including that frequency is measured in hertz, wavelength is the distance between peaks, and energy must be absorbed for electron excitation to higher orbital shapes like dumbbells. It concludes with a question calculating the frequency of a spectral line at 999nm.
Chemrev2
The document is a review of atomic theory, structure, and the mole concept. It asks questions about the law of definite proportions, discoveries of the cathode ray tube and electron, atomic models of J.J. Thompson and the gold foil experiment, the discovery of the nucleus, subatomic particles, isotopes, and relationships between moles, Avogadro's number, and molar mass.
C He Mreview
This document provides a chemistry review covering different units of measurement including density, length, mass, time and volume. It includes SI prefix conversions and sample problems calculating kilometers from miles, mass in grams from pounds, and liters of cola from ounces and cases. Sample density problems calculate the mass of a gold nugget given its volume and the density of gold, and the volume occupied by a given mass of carbon tetrachloride using its density.
Ph Yrev1
1) Susanna is 5.50 ft tall which is 167 cm. There are 4 quarts in a gallon of milk and 1 quart is 0.946 liters so 1 gallon is 3.785 liters. A 5 lb sack of potatoes has a mass of 2.27 kg. A 10K race is 10 km which is 6,214 feet. A 2 ton truck has a mass of 1,814 kg. A 3 L bottle of soda contains 180 teaspoons. If ants are 0.3 cm long, then 75 ants would be 22.5 cm or 0.225 meters long.
Econfig Pres
The document discusses electron configuration and the rules that govern how electrons fill atomic orbitals:
1) The Pauli Exclusion Principle states that each orbital can hold two electrons with opposite spins.
2) The Aufbau Principle states that electrons fill the lowest energy orbitals first, following the "lazy tenant rule."
3) Hund's Rule states that within a sublevel, one electron will occupy each orbital before pairing electrons, following the "empty bus seat rule."
Quantum Pres
The document summarizes the quantum model of the atom. It describes how electrons exhibit wave-like properties and have quantized wavelengths. The Heisenberg uncertainty principle states that it is impossible to know both the velocity and position of an electron at the same time. Schrodinger's wave equation defines quantized energy levels and the probability of finding an electron. Electrons occupy orbitals defined by four quantum numbers that specify the electron's unique "address" within the atom.
Cons Of Momentum Equations(2)
The document discusses the law of conservation of momentum through examples of rockets, toy vehicles crashing, and box cars colliding. It shows how to use the formula for momentum (mv) before and after interactions to calculate unknown velocities. For a rocket, the momentum of the rocket equals the momentum of the exhaust. A toy fire truck originally going 10 m/s hits a parked toy car, and the calculation shows the fire truck must be going 8 m/s after. When a 10 kg box car going 6 m/s crashes into a stationary 20 kg box car, sticking together their velocity is 2 m/s.
Quantum Pres
The document summarizes the quantum model of the atom. It describes how electrons exhibit wave-like properties and have quantized wavelengths. The Heisenberg uncertainty principle states that it is impossible to know both the velocity and position of an electron at the same time. Schrodinger's wave equation defines quantized energy levels and the probability of finding an electron. Electrons occupy orbitals defined by four quantum numbers that specify the electron's unique "address" within the atom.
Momentum Pres
This document discusses momentum and the conservation of momentum. It provides examples of calculating momentum using the formula momentum (p) = mass (m) x velocity (v). It also applies the law of conservation of momentum to example problems of objects colliding or a cannon firing, calculating the momentum before and after to find the unknown velocity.
Flametest
Different elements emit unique atomic line spectra colors when burned, due to electrons gaining and losing discrete energy levels and releasing photons of specific frequencies. Lithium burns with an orangish-yellow hue, demonstrating flame tests can distinguish elements based on their colored flames. Questions ask why chemicals have different colored flames, why heating is needed before light emission, and how metals create the color in salts.
Electronsreveiw
Waves and Electrons Review discusses wavelength, frequency, energy of waves including gamma rays and radio stations. It also covers emission spectrum and transitions between energy levels in atoms that produce different colors and types of electromagnetic radiation according to the Bohr model.
Bohr Model
The document discusses the Bohr model of the atom, which was inspired by Rutherford's model. According to the Bohr model, electrons can only exist in specific orbital energy levels and can only gain or lose fixed amounts of energy. As a result, only certain photons are produced. The energy of a photon depends on the difference in energy levels. Bohr's calculations matched the infrared, visible, and ultraviolet spectral lines for hydrogen. However, his calculations only worked for hydrogen and not other elements, which each have their own unique emission spectrum.
More from kitcoffeen (19)
Recently uploaded
Video Streaming: Then, Now, and in the Future
In his public lecture, Christian Timmerer provides insights into the fascinating history of video streaming, starting from its humble beginnings before YouTube to the groundbreaking technologies that now dominate platforms like Netflix and ORF ON. Timmerer also presents provocative contributions of his own that have significantly influenced the industry. He concludes by looking at future challenges and invites the audience to join in a discussion.
Taking AI to the Next Level in Manufacturing.pdf
Read Taking AI to the Next Level in Manufacturing to gain insights on AI adoption in the manufacturing industry, such as:
1. How quickly AI is being implemented in manufacturing.
2. Which barriers stand in the way of AI adoption.
3. How data quality and governance form the backbone of AI.
4. Organizational processes and structures that may inhibit effective AI adoption.
6. Ideas and approaches to help build your organization's AI strategy.
Let's Integrate MuleSoft RPA, COMPOSER, APM with AWS IDP along with Slack
Discover the seamless integration of RPA (Robotic Process Automation), COMPOSER, and APM with AWS IDP enhanced with Slack notifications. Explore how these technologies converge to streamline workflows, optimize performance, and ensure secure access, all while leveraging the power of AWS IDP and real-time communication via Slack notifications.
Infrastructure Challenges in Scaling RAG with Custom AI models
Building Retrieval-Augmented Generation (RAG) systems with open-source and custom AI models is a complex task. This talk explores the challenges in productionizing RAG systems, including retrieval performance, response synthesis, and evaluation. We’ll discuss how to leverage open-source models like text embeddings, language models, and custom fine-tuned models to enhance RAG performance. Additionally, we’ll cover how BentoML can help orchestrate and scale these AI components efficiently, ensuring seamless deployment and management of RAG systems in the cloud.
TrustArc Webinar - 2024 Global Privacy Survey
How does your privacy program stack up against your peers? What challenges are privacy teams tackling and prioritizing in 2024?
In the fifth annual Global Privacy Benchmarks Survey, we asked over 1,800 global privacy professionals and business executives to share their perspectives on the current state of privacy inside and outside of their organizations. This year’s report focused on emerging areas of importance for privacy and compliance professionals, including considerations and implications of Artificial Intelligence (AI) technologies, building brand trust, and different approaches for achieving higher privacy competence scores.
See how organizational priorities and strategic approaches to data security and privacy are evolving around the globe.
This webinar will review:
- The top 10 privacy insights from the fifth annual Global Privacy Benchmarks Survey
- The top challenges for privacy leaders, practitioners, and organizations in 2024
- Key themes to consider in developing and maintaining your privacy program
Your One-Stop Shop for Python Success: Top 10 US Python Development Providers
Simplify your search for a reliable Python development partner! This list presents the top 10 trusted US providers offering comprehensive Python development services, ensuring your project's success from conception to completion.
Essentials of Automations: The Art of Triggers and Actions in FME
In this second installment of our Essentials of Automations webinar series, we’ll explore the landscape of triggers and actions, guiding you through the nuances of authoring and adapting workspaces for seamless automations. Gain an understanding of the full spectrum of triggers and actions available in FME, empowering you to enhance your workspaces for efficient automation.
We’ll kick things off by showcasing the most commonly used event-based triggers, introducing you to various automation workflows like manual triggers, schedules, directory watchers, and more. Plus, see how these elements play out in real scenarios.
Whether you’re tweaking your current setup or building from the ground up, this session will arm you with the tools and insights needed to transform your FME usage into a powerhouse of productivity. Join us to discover effective strategies that simplify complex processes, enhancing your productivity and transforming your data management practices with FME. Let’s turn complexity into clarity and make your workspaces work wonders!
Uni Systems Copilot event_05062024_C.Vlachos.pdf
Unlocking Productivity: Leveraging the Potential of Copilot in Microsoft 365, a presentation by Christoforos Vlachos, Senior Solutions Manager – Modern Workplace, Uni Systems
Building Production Ready Search Pipelines with Spark and Milvus
Spark is the widely used ETL tool for processing, indexing and ingesting data to serving stack for search. Milvus is the production-ready open-source vector database. In this talk we will show how to use Spark to process unstructured data to extract vector representations, and push the vectors to Milvus vector database for search serving.
How to Get CNIC Information System with Paksim Ga.pptx
Pakdata Cf is a groundbreaking system designed to streamline and facilitate access to CNIC information. This innovative platform leverages advanced technology to provide users with efficient and secure access to their CNIC details.
Columbus Data & Analytics Wednesdays - June 2024
Columbus Data & Analytics Wednesdays, June 2024 with Maria Copot 20
“I’m still / I’m still / Chaining from the Block”
“An Outlook of the Ongoing and Future Relationship between Blockchain Technologies and Process-aware Information Systems.” Invited talk at the joint workshop on Blockchain for Information Systems (BC4IS) and Blockchain for Trusted Data Sharing (B4TDS), co-located with with the 36th International Conference on Advanced Information Systems Engineering (CAiSE), 3 June 2024, Limassol, Cyprus.
Microsoft - Power Platform_G.Aspiotis.pdf
Revolutionizing Application Development
with AI-powered low-code, presentation by George Aspiotis, Sr. Partner Development Manager, Microsoft
CAKE: Sharing Slices of Confidential Data on Blockchain
Presented at the CAiSE 2024 Forum, Intelligent Information Systems, June 6th, Limassol, Cyprus.
Synopsis: Cooperative information systems typically involve various entities in a collaborative process within a distributed environment. Blockchain technology offers a mechanism for automating such processes, even when only partial trust exists among participants. The data stored on the blockchain is replicated across all nodes in the network, ensuring accessibility to all participants. While this aspect facilitates traceability, integrity, and persistence, it poses challenges for adopting public blockchains in enterprise settings due to confidentiality issues. In this paper, we present a software tool named Control Access via Key Encryption (CAKE), designed to ensure data confidentiality in scenarios involving public blockchains. After outlining its core components and functionalities, we showcase the application of CAKE in the context of a real-world cyber-security project within the logistics domain.
Paper: https://doi.org/10.1007/978-3-031-61000-4_16
Generating privacy-protected synthetic data using Secludy and Milvus
During this demo, the founders of Secludy will demonstrate how their system utilizes Milvus to store and manipulate embeddings for generating privacy-protected synthetic data. Their approach not only maintains the confidentiality of the original data but also enhances the utility and scalability of LLMs under privacy constraints. Attendees, including machine learning engineers, data scientists, and data managers, will witness first-hand how Secludy's integration with Milvus empowers organizations to harness the power of LLMs securely and efficiently.
Climate Impact of Software Testing at Nordic Testing Days
My slides at Nordic Testing Days 6.6.2024
Climate impact / sustainability of software testing discussed on the talk. ICT and testing must carry their part of global responsibility to help with the climat warming. We can minimize the carbon footprint but we can also have a carbon handprint, a positive impact on the climate. Quality characteristics can be added with sustainability, and then measured continuously. Test environments can be used less, and in smaller scale and on demand. Test techniques can be used in optimizing or minimizing number of tests. Test automation can be used to speed up testing.
Mind map of terminologies used in context of Generative AI
Mind map of common terms used in context of Generative AI.
HCL Notes and Domino License Cost Reduction in the World of DLAU
Webinar Recording: https://www.panagenda.com/webinars/hcl-notes-and-domino-license-cost-reduction-in-the-world-of-dlau/
The introduction of DLAU and the CCB & CCX licensing model caused quite a stir in the HCL community. As a Notes and Domino customer, you may have faced challenges with unexpected user counts and license costs. You probably have questions on how this new licensing approach works and how to benefit from it. Most importantly, you likely have budget constraints and want to save money where possible. Don’t worry, we can help with all of this!
We’ll show you how to fix common misconfigurations that cause higher-than-expected user counts, and how to identify accounts which you can deactivate to save money. There are also frequent patterns that can cause unnecessary cost, like using a person document instead of a mail-in for shared mailboxes. We’ll provide examples and solutions for those as well. And naturally we’ll explain the new licensing model.
Join HCL Ambassador Marc Thomas in this webinar with a special guest appearance from Franz Walder. It will give you the tools and know-how to stay on top of what is going on with Domino licensing. You will be able lower your cost through an optimized configuration and keep it low going forward.
These topics will be covered
- Reducing license cost by finding and fixing misconfigurations and superfluous accounts
- How do CCB and CCX licenses really work?
- Understanding the DLAU tool and how to best utilize it
- Tips for common problem areas, like team mailboxes, functional/test users, etc
- Practical examples and best practices to implement right away
Driving Business Innovation: Latest Generative AI Advancements & Success Story
Are you ready to revolutionize how you handle data? Join us for a webinar where we’ll bring you up to speed with the latest advancements in Generative AI technology and discover how leveraging FME with tools from giants like Google Gemini, Amazon, and Microsoft OpenAI can supercharge your workflow efficiency.
During the hour, we’ll take you through:
Guest Speaker Segment with Hannah Barrington: Dive into the world of dynamic real estate marketing with Hannah, the Marketing Manager at Workspace Group. Hear firsthand how their team generates engaging descriptions for thousands of office units by integrating diverse data sources—from PDF floorplans to web pages—using FME transformers, like OpenAIVisionConnector and AnthropicVisionConnector. This use case will show you how GenAI can streamline content creation for marketing across the board.
Ollama Use Case: Learn how Scenario Specialist Dmitri Bagh has utilized Ollama within FME to input data, create custom models, and enhance security protocols. This segment will include demos to illustrate the full capabilities of FME in AI-driven processes.
Custom AI Models: Discover how to leverage FME to build personalized AI models using your data. Whether it’s populating a model with local data for added security or integrating public AI tools, find out how FME facilitates a versatile and secure approach to AI.
We’ll wrap up with a live Q&A session where you can engage with our experts on your specific use cases, and learn more about optimizing your data workflows with AI.
This webinar is ideal for professionals seeking to harness the power of AI within their data management systems while ensuring high levels of customization and security. Whether you're a novice or an expert, gain actionable insights and strategies to elevate your data processes. Join us to see how FME and AI can revolutionize how you work with data!
Recently uploaded (20)
Let's Integrate MuleSoft RPA, COMPOSER, APM with AWS IDP along with Slack
Let's Integrate MuleSoft RPA, COMPOSER, APM with AWS IDP along with Slack
Infrastructure Challenges in Scaling RAG with Custom AI models
Infrastructure Challenges in Scaling RAG with Custom AI models
Your One-Stop Shop for Python Success: Top 10 US Python Development Providers
Your One-Stop Shop for Python Success: Top 10 US Python Development Providers
Essentials of Automations: The Art of Triggers and Actions in FME
Essentials of Automations: The Art of Triggers and Actions in FME
Building Production Ready Search Pipelines with Spark and Milvus
Building Production Ready Search Pipelines with Spark and Milvus
How to Get CNIC Information System with Paksim Ga.pptx
How to Get CNIC Information System with Paksim Ga.pptx
CAKE: Sharing Slices of Confidential Data on Blockchain
CAKE: Sharing Slices of Confidential Data on Blockchain
Generating privacy-protected synthetic data using Secludy and Milvus
Generating privacy-protected synthetic data using Secludy and Milvus
Climate Impact of Software Testing at Nordic Testing Days
Climate Impact of Software Testing at Nordic Testing Days
Mind map of terminologies used in context of Generative AI
Mind map of terminologies used in context of Generative AI
HCL Notes and Domino License Cost Reduction in the World of DLAU
HCL Notes and Domino License Cost Reduction in the World of DLAU
Driving Business Innovation: Latest Generative AI Advancements & Success Story
Driving Business Innovation: Latest Generative AI Advancements & Success Story
Physicsjeopardy
- 1. 2 pt 3 pt 4 pt 5pt 1 pt 2 pt 3 pt 4 pt 5 pt 1 pt 2pt 3 pt 4pt 5 pt 1pt 2pt 3 pt 4 pt 5 pt 1 pt 2 pt 3 pt 4pt 5 pt 1pt Gravity and Projectiles Potpourri Newton’s 1st Newton’s 2nd Newton’s 3rd
- 2. Why is it important that a satellite be above earth’s atmosphere?
- 3. So it won’t encounter air resistance
- 4. At what angle should a slingshot be oriented to achieve maximum distance?
- 5. 45 degrees
- 6. What is the acceleration of Gravity? (Rounded to the nearest tenth)
- 7. 9.8 m/s
- 8. A ball is thrown straight up at 30m/s, about how long will it be in the air?
- 9. 6 seconds
- 10. Given d=1/2at 2 How far will an object have fallen if it was dropped from a plane 16 seconds ago?
- 11. 480m
- 12. The kilogram is a measure of an object’s:
- 13. Mass
- 14. This gives you both the magnitude and direction of velocity
- 15. What is a velocity vector?
- 16. This force ensures that an object, whether rolled or thrown will always come to a stop.
- 18. Who is the coolest teacher ever?
- 19. Mr. Coffeen
- 20. How much does one kilogram weigh in Newtons?
- 21. 9.8N or 10N
- 22. This is the force that is explained by Newton’s First Law
- 23. What is inertia?
- 24. Inertia applies to bodies at rest and:
- 25. Bodies in constant motion
- 26. If a body has twice the inertia of another body, it also has twice the_____
- 27. Mass of the other body
- 28. A large man and a small woman are on a train that makes a sudden stop. The woman falls forward but the man keeps his footing. Who had more inertia?
- 29. The large man
- 30. Does a bowling ball have more inertia on the Earth or on the Moon?
- 31. The same both places
- 32. What equation do we use to describe Newton’s Second Law?
- 33. F=ma
- 34. 10kg brick and a 1kg brick are dropped in a vacuum, the force of gravity on the 10kg brick is:
- 35. 10 times as much
- 36. An object is pulled northward at 20N and southward at 15N. What magnitude of the net force?
- 37. 5N
- 38. A 1000kg truck is accelerated at 8m/s/s, how much force was applied to do so?
- 39. 8000N
- 40. Convert this equation into the force gravity exerts on earth: F=ma
- 41. F=ga Or F=10a Or F=9.8a
- 42. Paraphrase Newton’s Third Law
- 43. Every action has an equal and opposite reaction
- 44. A high school student hits a nail with a hammer. During the collision there is a force on which object?
- 45. Both nail and hammer
- 46. A boxer swings as hard as he can at a helium balloon then equally hard at a punching bag. Which object did he hit with more force?
- 47. The punching bag
- 48. An archer shoots an arrow. Consider the action force to be the bowstring pushing against the arrow. The reaction force is:
- 49. The arrow pushing against the bowstring
- 50. A rocket is able to propel itself in in the vacuum of space by firing its engines. The force that propels the rocket is:
- 51. The exhaust gasses rushing away from the ship