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Circular Motion PPT
Circular Motion PPT

... To find the MAGNITUDES of each we have: ...
AP Physics C - Circular Motion
AP Physics C - Circular Motion

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Speed, Velocity, Acceleration, and Force

... If the forces are in the same direction, all you have to do is add them. The net force will be in that same direction. If the forces are pointing in opposite directions: 1. Take the difference. 2. The net force will be in the direction of the larger force. What is the difference between a balanced a ...
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Tue Sep 21

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Projectile Motion
Projectile Motion

... any object that is launched with an initial velocity and continues to move; affected only by the force of gravity.  Trajectory: the path a projectile follows.  Usually parabolic  Range: horizontal distance covered by a projectile  Height: the maximum vertical distance reached by a projectile ...
Ch. 4,5,6 ------------------- Forces, Circular Motion, Energy
Ch. 4,5,6 ------------------- Forces, Circular Motion, Energy

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Worksheet - Uniform Circular Motion File

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CH-5 Lecture - Chemistry at Winthrop University

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FA#5--Rotational Dynamics I FA#5

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Gravity and Motion

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REVISION: NEWTON`S LAWS 25 MARCH 2014 Lesson Description

... The SI units of acceleration are m.s . Acceleration is a vector quantity. When an object speeds up in the positive direction, acceleration is positive. When an object slows down while moving in the positive direction, the acceleration is negative (opposite to the direction of ...
1. An 80 kg water skier is being pulled by a boat with a force of 220
1. An 80 kg water skier is being pulled by a boat with a force of 220

... 1. An 80 kg water skier is being pulled by a boat with a force of 220 N causing the skier to accelerate at 1.8 m/s2. Find the drag force on the skier. 2. A 2000 kg car is slowed down uniformly from 20 m/s to 5 m/s in 4 seconds. Determine the average net force on the car during this time, and how far ...
Universal Law of Gravitation
Universal Law of Gravitation

... 5. A 1 kg object is located at a distance of 1.7 x106 m from the center of a larger object whose mass is 7.4 x 1022 kg. a. What is the size of the force acting on the smaller object? 1.71 N b. What is the size of the force acting on the larger object? 1.71 N c. What is the acceleration of the smalle ...
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Newton`s Laws of Motion Practice Test General Physics

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Second practice midetrm key (Word document)

... B. Assuming the Force Sensor was tared properly what value you would expect to read from it in the scenario shown above? Explain/show work Would be half weight .5*(.2586)*(9.8) = 1.267 N C. How does one Tare the Force Sensor? What does that do? How: press button on side (when nothing) is pulling or ...
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Uniform circular motion (PPT)

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Newton’s 2nd Law

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Pioneer anomaly

The Pioneer anomaly or Pioneer effect was the observed deviation from predicted accelerations of the Pioneer 10 and Pioneer 11 spacecraft after they passed about 20 astronomical units (3×109 km; 2×109 mi) on their trajectories out of the Solar System. The apparent anomaly was a matter of tremendous interest for many years, but has been subsequently explained by an anisotropic radiation pressure caused by the spacecraft's heat loss.Both Pioneer spacecraft are escaping the Solar System, but are slowing under the influence of the Sun's gravity. Upon very close examination of navigational data, the spacecraft were found to be slowing slightly more than expected. The effect is an extremely small acceleration towards the Sun, of 6990874000000000000♠(8.74±1.33)×10−10 m/s2, which is equivalent to slowly accelerating to a velocity of 1 kilometre per hour (0.6 mph) over a period of ten years. The two spacecraft were launched in 1972 and 1973 and the anomalous acceleration was first noticed as early as 1980, but not seriously investigated until 1994. The last communication with either spacecraft was in 2003, but analysis of recorded data continues.Various explanations, both of spacecraft behavior and of gravitation itself, were proposed to explain the anomaly. Over the period 1998–2012, one particular explanation became accepted. The spacecraft, which are surrounded by an ultra-high vacuum and are each powered by a radioisotope thermoelectric generator (RTG), can shed heat only via thermal radiation. If, due to the design of the spacecraft, more heat is emitted in a particular direction—what is known as a radiative anisotropy—then the spacecraft would accelerate slightly in the direction opposite of the excess emitted radiation due to radiation pressure. Because this force is due to the recoil of thermal photons, it is also called the thermal recoil force. If the excess radiation and attendant radiation pressure were pointed in a general direction opposite the Sun, the spacecraft's velocity away from the Sun would be decelerating at a greater rate than could be explained by previously recognized forces, such as gravity and trace friction, due to the interplanetary medium (imperfect vacuum).By 2012 several papers by different groups, all reanalyzing the thermal radiation pressure forces inherent in the spacecraft, showed that a careful accounting of this explains the entire anomaly, and thus the cause was mundane and did not point to any new phenomena or need for a different physical paradigm. The most detailed analysis to date, by some of the original investigators, explicitly looks at two methods of estimating thermal forces, then states ""We find no statistically significant difference between the two estimates and conclude that once the thermal recoil force is properly accounted for, no anomalous acceleration remains.""
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