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lin eq
lin eq

SolvingLinearSystemspt1
SolvingLinearSystemspt1

1 - JustAnswer
1 - JustAnswer

Class Worked Example
Class Worked Example

Chapter 9.5--Equations Containing Fractions Chapter 9.5
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... archway. To make it look interesting, she has decided to put the banner on an angle. She sets the banner along a line defined by the linear equation y 5 0.24x  7.2, with x representing the horizontal distance and y the vertical distance, in metres, from one foot of the archway. The archway is model ...
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Kristy`s Garden - Standards Toolkit

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1.) Do I Exist? You have to be able to explain why or why not!

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Polar Coordinates: Instead of the rectangular coordinate system (x, y

... Equations in Polar Form: In rectangular coordinate, we know that the equations x = 2 or y = 3 are equations of vertical and horizontal lines, respectively. What do the equations r = 2 and θ = 3 in polar coordinate represent? Note that in the rectangular equation, x = 2, y is a free variable, meanin ...
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... 3. Describe two ways to verify that the quadrilateral formed is a parallelogram. Answers may vary. An example is provided. One way to verify that the resulting quadrilateral is a parallelogram is to compare the slopes of the line representing the sides. If both pairs of the opposite sides have the s ...
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3.2

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Schwarzschild geodesics

In general relativity, the geodesics of the Schwarzschild metric describe the motion of particles of infinitesimal mass in the gravitational field of a central fixed mass M. The Schwarzschild geodesics have been pivotal in the validation of the Einstein's theory of general relativity. For example, they provide quite accurate predictions of the anomalous precession of the planets in the Solar System, and of the deflection of light by gravity.The Schwarzschild geodesics pertain only to the motion of particles of infinitesimal mass m, i.e., particles that do not themselves contribute to the gravitational field. However, they are highly accurate provided that m is many-fold smaller than the central mass M, e.g., for planets orbiting their sun. The Schwarzschild geodesics are also a good approximation to the relative motion of two bodies of arbitrary mass, provided that the Schwarzschild mass M is set equal to the sum of the two individual masses m1 and m2. This is important in predicting the motion of binary stars in general relativity.
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