Answer to Question #129591 in Algebra for Sphesihle Zuma

Question #129591
QUESTION 1
1.1. Define the following concepts and give an example in each case.
1.1.1. Ratio (3)
1.1.2. Direct proportion (3)
1.1.3. Indirect proportion
1
Expert's answer
2020-08-16T20:27:24-0400

1.1.1. A ratio, which is a comparison of two numbers by division, is the quotient obtained when the first number is divided by the second, nonzero number.

In general, the ratio of "a" to "b" can be expressed as


"{a \\over b}\\ \\ \\text{or}\\ \\ a \\div b \\ \\ \\text{or}\\ \\ a : b"

To find the ratio of two quantities, both quantities must be expressed in the same unit of measure before their quotient is determined.

The ratio has no unit of measure.

Example: sine ratio is the ratio of the length of the opposite side divided by the length of the hypotenuse. 


1.1.2. Two values "x" and "y" are directly proportional to each other when the ratio "x: y" or "\\dfrac{x}{y}"  is a constant (i.e. always remains the same). This would mean that "x" and "y" will either increase together or decrease together by an amount that would not change the ratio.

Example: If an object travels at a constant speed, then the distance traveled is directly proportional to the time spent traveling, with the speed being the constant of proportionality. 


1.1.3. Two values "x" and "y" are inversely proportional (indirect proportion)to each other when their product "xy" is a constant (always remains the same). This means that when "x" increases "y" will decrease, and vice versa, by an amount such that "xy" remains the same.

Example: Newton's law of universal gravitation states that every particle attracts every other particle in the universe with a force that is directly proportional to the product of their masses and inversely proportional to the square of the distance between their centers.


"F_{gr}=G\\dfrac{m_1m_2}{r^2}"

where "F_{gr}" is the gravitational force acting between two objects, "m_1" and "m_2" are the masses of the objects, "r" is the distance between the centers of their masses, and "G" is the gravitational constant.



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