“The Government Roles” WebQuest Lesson Plan
... Explore Newton's First Law - The Law of InertiaTo better understand Newton’s First Law, you will need a toy car, and a partner. Think about this: An object in motion stays in motion. What does this mean? Have about five feet of space between you and your partner. Now facing each other, roll the car ...
... Explore Newton's First Law - The Law of InertiaTo better understand Newton’s First Law, you will need a toy car, and a partner. Think about this: An object in motion stays in motion. What does this mean? Have about five feet of space between you and your partner. Now facing each other, roll the car ...
Super Giant
... Explain why the moon revolves around the Earth instead of the Sun. Even though the moon is larger than Pluto, which DOES revolve around the Sun, The moon revolves around the Earth because it is CLOSER to the Earth. The two factors that determine the force of gravity are mass and distance. What relat ...
... Explain why the moon revolves around the Earth instead of the Sun. Even though the moon is larger than Pluto, which DOES revolve around the Sun, The moon revolves around the Earth because it is CLOSER to the Earth. The two factors that determine the force of gravity are mass and distance. What relat ...
Ch 5 Review Questions
... This formula shows that both the size of the force and the mass of the object itself affect the object’s acceleration, or change in velocity (speed or direction). a. b. c. d. ...
... This formula shows that both the size of the force and the mass of the object itself affect the object’s acceleration, or change in velocity (speed or direction). a. b. c. d. ...
Microsoft Powerpoint
... forces are all manifestations of the electromagnetic force They all are the result of attractive (and repulsive) forces of atoms and molecules within an object (normal and tension) or at the interface of two objects Applications of Newton’s 2nd Law Equilibrium – an object which has zero accelera ...
... forces are all manifestations of the electromagnetic force They all are the result of attractive (and repulsive) forces of atoms and molecules within an object (normal and tension) or at the interface of two objects Applications of Newton’s 2nd Law Equilibrium – an object which has zero accelera ...
FORCES IN ONE DIMENSION
... A 1.0-kg mass at rest is suspended from a spring scale. The direction of positive forces that are acting or could act on the 1.0-kg mass are shown to the right. 9. The 1.0-kg mass and spring scale are being lifted at a constant speed. The net force on the mass is ____ . a. 0 N ...
... A 1.0-kg mass at rest is suspended from a spring scale. The direction of positive forces that are acting or could act on the 1.0-kg mass are shown to the right. 9. The 1.0-kg mass and spring scale are being lifted at a constant speed. The net force on the mass is ____ . a. 0 N ...
FORCES AND NEWTON`S LAWS OF MOTION
... property of matter and does not change as an object is moved from one location to another while • Weight is the gravitational force acting on an object and can vary, depending on how far the object is above the earth’s surface or whether it is located near another body such as the moon. ...
... property of matter and does not change as an object is moved from one location to another while • Weight is the gravitational force acting on an object and can vary, depending on how far the object is above the earth’s surface or whether it is located near another body such as the moon. ...
Torque Web Quest
... – Solid cylinder: I = (1/2) MR2 (use for part II in lab) – Hollow sphere: I = (2/3) MR2 – Solid sphere: I = (2/5) MR2 ...
... – Solid cylinder: I = (1/2) MR2 (use for part II in lab) – Hollow sphere: I = (2/3) MR2 – Solid sphere: I = (2/5) MR2 ...
p250c05
... degrees from overhead in Alexandria. (see astro 03f14.jpg) Using the known distance between the cities, he was able to determine the radius of the Earth. Using the distance of 770 km between these cities, calculate the radius of the earth. ...
... degrees from overhead in Alexandria. (see astro 03f14.jpg) Using the known distance between the cities, he was able to determine the radius of the Earth. Using the distance of 770 km between these cities, calculate the radius of the earth. ...
Introduction to Mechanics
... Forces are influences on a body or system which, acting alone, would cause the motion of that body or system to change. A system or body at rest and then subjected to a force will start to move. To work with forces we need to know the magnitude (size), direction and the point of application of the f ...
... Forces are influences on a body or system which, acting alone, would cause the motion of that body or system to change. A system or body at rest and then subjected to a force will start to move. To work with forces we need to know the magnitude (size), direction and the point of application of the f ...
Chapter 17
... A. From radio waves reflected of the galactic nucleus. B. From its Doppler shift C. From the "fixed basis" of globular clusters in the galactic halo. D. From the proper motions of nearby open clusters. 16. The reason we can use RR-Lyrae stars to find our distance from the Galaxy's center is: A. of t ...
... A. From radio waves reflected of the galactic nucleus. B. From its Doppler shift C. From the "fixed basis" of globular clusters in the galactic halo. D. From the proper motions of nearby open clusters. 16. The reason we can use RR-Lyrae stars to find our distance from the Galaxy's center is: A. of t ...
Problem Solving Tip Sheet
... There are certain types of collisions which are special. A collision (not an object) can be characterized as completely inelastic, elastic, explosive, or none of these. If the collision is completely inelastic, then the velocities of all objects will be the same after the collision (the objects stic ...
... There are certain types of collisions which are special. A collision (not an object) can be characterized as completely inelastic, elastic, explosive, or none of these. If the collision is completely inelastic, then the velocities of all objects will be the same after the collision (the objects stic ...
Newton`s Laws and Force Review
... d. 9.8 N e. none of the above 23. An apple weighs 1 N. When held at rest on top of your head, the net force on the apple is _____. a. 0 N b. 0.1 N c. 1 N d. 9.8 N e. none of the above 24. A girls pulls a 10 kg wagon with a net force of 30 N. What is the wagon’s acceleration? a. 0.3 m/s2 b. 3.0 m/s2 ...
... d. 9.8 N e. none of the above 23. An apple weighs 1 N. When held at rest on top of your head, the net force on the apple is _____. a. 0 N b. 0.1 N c. 1 N d. 9.8 N e. none of the above 24. A girls pulls a 10 kg wagon with a net force of 30 N. What is the wagon’s acceleration? a. 0.3 m/s2 b. 3.0 m/s2 ...
The Classification of Galaxies By Daniel Underwood Contents The
... Lenticular galaxies appear to be intermediate between elliptical and spiral galaxies, where their structure shows an elliptical style that is more elongated, where 10e is greater than 7, although spiral galaxy features may be present, if very slightly. These galaxies are denoted by “SA0” or “SB0”. ...
... Lenticular galaxies appear to be intermediate between elliptical and spiral galaxies, where their structure shows an elliptical style that is more elongated, where 10e is greater than 7, although spiral galaxy features may be present, if very slightly. These galaxies are denoted by “SA0” or “SB0”. ...
AP Physics – Gravity and Circular Motion
... What is the source of the centripetal force required to make the earth revolve around the sun? This is where the apple falling on Newton story fits in. Before Newton no one could explain the orbits of the planets and moons. Newton, the story goes, was relaxing under an apple tree pondering the probl ...
... What is the source of the centripetal force required to make the earth revolve around the sun? This is where the apple falling on Newton story fits in. Before Newton no one could explain the orbits of the planets and moons. Newton, the story goes, was relaxing under an apple tree pondering the probl ...
Walker Chapter 5 (Newton`s Laws)
... 5-2 Newton’s First Law of Motion • In order to change the velocity of an object— magnitude or direction—a net force is required. • An inertial reference frame is one in which the first law is true. The surface of the earth is a good approximation to an inertial frame of reference. Accelerating refe ...
... 5-2 Newton’s First Law of Motion • In order to change the velocity of an object— magnitude or direction—a net force is required. • An inertial reference frame is one in which the first law is true. The surface of the earth is a good approximation to an inertial frame of reference. Accelerating refe ...
Question paper
... A area under a displacement-time graph B area under a force-time graph C gradient of a displacement-time graph D gradient of an acceleration-time graph (Total for Question 9 = 1 mark) 10 A freely falling object on Earth has a speed of 5.0 m s–1. After falling a further 20 m its speed is A 15 m s–1 B ...
... A area under a displacement-time graph B area under a force-time graph C gradient of a displacement-time graph D gradient of an acceleration-time graph (Total for Question 9 = 1 mark) 10 A freely falling object on Earth has a speed of 5.0 m s–1. After falling a further 20 m its speed is A 15 m s–1 B ...
Modified Newtonian dynamics
In physics, modified Newtonian dynamics (MOND) is a theory that proposes a modification of Newton's laws to account for observed properties of galaxies. Created in 1983 by Israeli physicist Mordehai Milgrom, the theory's original motivation was to explain the fact that the velocities of stars in galaxies were observed to be larger than expected based on Newtonian mechanics. Milgrom noted that this discrepancy could be resolved if the gravitational force experienced by a star in the outer regions of a galaxy was proportional to the square of its centripetal acceleration (as opposed to the centripetal acceleration itself, as in Newton's Second Law), or alternatively if gravitational force came to vary inversely with radius (as opposed to the inverse square of the radius, as in Newton's Law of Gravity). In MOND, violation of Newton's Laws occurs at extremely small accelerations, characteristic of galaxies yet far below anything typically encountered in the Solar System or on Earth.MOND is an example of a class of theories known as modified gravity, and is an alternative to the hypothesis that the dynamics of galaxies are determined by massive, invisible dark matter halos. Since Milgrom's original proposal, MOND has successfully predicted a variety of galactic phenomena that are difficult to understand from a dark matter perspective. However, MOND and its generalisations do not adequately account for observed properties of galaxy clusters, and no satisfactory cosmological model has been constructed from the theory.