Her Body in Motion

"As a weather vane she will be a strong sight: her body will come with the wind." - Emmanuel von Shack, Educator, and ASL user

How do you contact the carved body? Let's listen to international experts, leading authorities, nova from a unique perspective on gestures, facial expressions and gesture languages.

Inference: From the attribute point of view, if the problem location is moving, the body moving from a particular location is only a part of the movement of the body. The complete and actual movement of the body involves movement relative to the movement position and adds motion that may be in the field to the ground. If the place moves relative to the place of movement, you need to add a move of the place. Unless you retreat indefinitely, the sum must end with a motion relative to the stationary position.

Every movement is associated with a specific reference frame. To say that the body is stationary means that it is not moving, that is just as it is described as the frame of reference moving with the body. For example, an object on the surface of the earth may appear to be stationary, because the observer is also on the surface of the earth. Along with the human body and the observer, the earth itself orbits around the sun and rotates around its own axis. Normally, the movement of the body follows the Newton's kinetic law. However, the relative speed must be used to handle motion close to light speed and quantum mechanics must be used to handle the motion of very small objects such as electrons.

Based on classical mechanics, it can be considered that the movement of the body can be described as a combination of free (or inertial) movement and deviation from such free movement. This deviation is caused by external force acting on the body according to Newton's second motion law. This indicates that the net force acting on the body is equal to the mass (inertia) of the body multiplied by its acceleration. The preferred inertial motion is related to the geometric shape of space and time. In a standard reference system of classical mechanics, an object in free motion moves linearly at a constant speed. In contemporary terminology, those paths are geodesic, straight lines that bend time and space.