Create natural-looking motion without the need for complex calculations using preset behaviors like Gravity, Throw, and Vortex. Use Text behaviors that animate letters, words, or lines across the screen. Or apply the Overshoot behavior to easily create spring-loaded animations. You can even combine behaviors for more advanced motion animations.

Quickly animate text on or off the screen by choosing from more than 100 behaviors including Type On, Blur Out, and Text-on-a-Path, which sets your text in motion on a trajectory that angles, bends, or twists. You can also create unique animations by moving letters just where you want them.


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In physics, motion is when an object changes its position with respect to a reference point in a given time. Motion is mathematically described in terms of displacement, distance, velocity, acceleration, speed, and frame of reference to an observer, measuring the change in position of the body relative to that frame with a change in time. The branch of physics describing the motion of objects without reference to their cause is called kinematics, while the branch studying forces and their effect on motion is called dynamics.

Motion applies to various physical systems: objects, bodies, matter particles, matter fields, radiation, radiation fields, radiation particles, curvature, and space-time. One can also speak of the motion of images, shapes, and boundaries. In general, the term motion signifies a continuous change in the position or configuration of a physical system in space. For example, one can talk about the motion of a wave or the motion of a quantum particle, where the configuration consists of the probabilities of the wave or particle occupying specific positions.

In physics, the motion of massive bodies is described through two related sets of laws of mechanics. Classical mechanics for super atomic (larger than an atom) objects (such as cars, projectiles, planets, cells, and humans) and quantum mechanics for atomic and sub-atomic objects (such as helium, protons, and electrons). Historically, Newton and Euler formulated three laws of classical mechanics:

Classical mechanics is used for describing the motion of macroscopic objects moving at speeds significantly slower than the speed of light, from projectiles to parts of machinery, as well as astronomical objects, such as spacecraft, planets, stars, and galaxies. It produces very accurate results within these domains and is one of the oldest and largest scientific descriptions in science, engineering, and technology.

Classical mechanics is fundamentally based on Newton's laws of motion. These laws describe the relationship between the forces acting on a body and the motion of that body. They were first compiled by Sir Isaac Newton in his work Philosophi Naturalis Principia Mathematica, which was first published on July 5, 1687. Newton's three laws are:

Newton's three laws of motion were the first to accurately provide a mathematical model for understanding orbiting bodies in outer space. This explanation unified the motion of celestial bodies and the motion of objects on Earth.

In addition to describing the motion of atomic level phenomena, quantum mechanics is useful in understanding some large-scale phenomena such as superfluidity, superconductivity, and biological systems, including the function of smell receptors and the structures of protein.[8]

Spacetime (the fabric of the universe) is expanding, meaning everything in the universe is stretching, like a rubber band. This motion is the most obscure as it is not physical motion, but rather a change in the very nature of the universe. The primary source of verification of this expansion was provided by Edwin Hubble who demonstrated that all galaxies and distant astronomical objects were moving away from Earth, known as Hubble's law, predicted by a universal expansion.[10]

The Milky Way Galaxy is moving through space and many astronomers believe the velocity of this motion to be approximately 600 kilometres per second (1,340,000 mph) relative to the observed locations of other nearby galaxies. Another reference frame is provided by the Cosmic microwave background. This frame of reference indicates that the Milky Way is moving at around 582 kilometres per second (1,300,000 mph).[11][failed verification]

The Milky Way is rotating around its dense Galactic Center, thus the Sun is moving in a circle within the galaxy's gravity. Away from the central bulge, or outer rim, the typical stellar velocity is between 210 and 240 kilometres per second (470,000 and 540,000 mph).[12] All planets and their moons move with the Sun. Thus, the Solar System is in motion.

According to the laws of thermodynamics, all particles of matter are in constant random motion as long as the temperature is above absolute zero. Thus the molecules and atoms which make up the human body are vibrating, colliding, and moving. This motion can be detected as temperature; higher temperatures, which represent greater kinetic energy in the particles, feel warm to humans who sense the thermal energy transferring from the object being touched to their nerves. Similarly, when lower temperature objects are touched, the senses perceive the transfer of heat away from the body as a feeling of cold.[24]

Some motion appears to an observer to exceed the speed of light. Bursts of energy moving out along the relativistic jets emitted from these objects can have a proper motion that appears greater than the speed of light. All of these sources are thought to contain a black hole, responsible for the ejection of mass at high velocities. Light echoes can also produce apparent superluminal motion.[29] This occurs owing to how motion is often calculated at long distances; oftentimes calculations fail to account for the fact that the speed of light is finite. When measuring the movement of distant objects across the sky, there is a large time delay between what has been observed and what has occurred, due to the large distance the light from the distant object has to travel to reach us. The error in the above naive calculation comes from the fact that when an object has a component of velocity directed towards the Earth, as the object moves closer to the Earth that time delay becomes smaller. This means that the apparent speed as calculated above is greater than the actual speed. Correspondingly, if the object is moving away from the Earth, the above calculation underestimates the actual speed.[30]

Set your waves in motion and get frizz under control with this weightless, highly-absorbent, curl enhancing lotion. MOTION.LOTION is the secret to defining loose, soft waves with flexible hold in long or fine hair. The added bonus of super-charged nourishing oils boost natural-looking shine as you twist and twirl into hair.

The NGA-West2 ground motion database includes a very large set of ground motions recorded in worldwide shallow crustal earthquakes in active tectonic regimes. The database has one of the most comprehensive sets of meta-data, including different distance measure, various site characterizations, earthquake source data, etc. The current version of the database is similar to the NGA-West2 database, which was used to develop the 2014 NGA-West2 ground motion models (GMMs). peer.berkeley.edu/ngawest2

The objective of NGA-East is to develop a new ground motion characterization (GMC) model for the Central and Eastern North-American (CENA) region. The GMC model consists in a set of new ground motion models (GMMs) for median and standard deviation of ground motions (GMs) and their associated weights in the logic-trees for use in probabilistic seismic hazard analyses (PSHA). peer.berkeley.edu/ngaeast

The PEER NGA strong-motion databases, the associated flatfiles, reports, and products are subject to future revisions as a result of the review process, as new information is obtained, or as new interpretations are made.

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FutureProof provides Ringling College students with a professional motion design conference experience. This unique, week-long event offers a variety of presentations, workshops, and activities all designed to prepare students for a smooth transition from the classroom experience into their future careers. The 2022 Conference features speakers from Scholar, Nickelodeon, BUCK, FutureDeluxe, Hornet, Telemundo, Hue&Cry.

We believe in empowering our clients to live life in motion. Find out how our services can help you recover from an injury, improve your mobility, or even make you a stronger athlete. With our convenient locations and experienced professionals, MOTION is here to help.

Alexandria is a desirable location to live, work and play. The City owns many of the premier historic sites in Alexandria and it is charged with the conservation, interpretation and promotion of these links to the past.

One of the last steps a prosecutor takes before trial is to respond to or file motions. A motion is an application to the court made by the prosecutor or defense attorney, requesting that the court make a decision on a certain issue before the trial begins. The motion can affect the trial, courtroom, defendants, evidence, or testimony.

Since launching the Utah Artificial Arm, Fillauer Motion Control has developed a number of innovative products to help improve the freedom, motion and lifestyle of its clients. Learn more about our product lines by choosing one of the links.

A motion is a formal request to a judge to make a ruling or take some other action during a lawsuit. A motion does not start a lawsuit, but rather brings a limited, contested issue in a case before the court for a decision. 2351a5e196

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