Direct proportionality in the context of "Linear acceleration"

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⭐ Core Definition: Direct proportionality

In mathematics, two sequences of numbers, often experimental data, are proportional or directly proportional if their corresponding elements have a constant ratio. The ratio is called coefficient of proportionality (or proportionality constant) and its reciprocal is known as constant of normalization (or normalizing constant). Two sequences are inversely proportional if corresponding elements have a constant product.

Two functions and are proportional if their ratio is a constant function.

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Direct proportionality in the context of Acceleration

In mechanics, acceleration is the rate of change of the velocity of an object with respect to time. Acceleration is one of several components of kinematics, the study of motion. Accelerations are vector quantities (in that they have magnitude and direction). The orientation of an object's acceleration is given by the orientation of the net force acting on that object. The magnitude of an object's acceleration, as described by Newton's second law, is the combined effect of two causes:

The SI unit for acceleration is metre per second squared (m⋅s, ).

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Direct proportionality in the context of Period-luminosity relation

In astronomy, a period-luminosity relation is a relationship linking the luminosity of pulsating variable stars with their pulsation period.The best-known relation is the direct proportionality law holding for Classical Cepheid variables, sometimes called the Leavitt Law. Discovered in 1908 by Henrietta Swan Leavitt, the relation established Cepheids as foundational indicators of cosmic benchmarks for scaling galactic and extragalactic distances.The physical model explaining the Leavitt's law for classical cepheids is called kappa mechanism.

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