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In this section, you will:
  • Evaluate  2 × 2  determinants.
  • Use Cramer’s Rule to solve a system of equations in two variables.
  • Evaluate  3 × 3  determinants.
  • Use Cramer’s Rule to solve a system of three equations in three variables.
  • Know the properties of determinants.

We have learned how to solve systems of equations in two variables and three variables, and by multiple methods: substitution, addition, Gaussian elimination, using the inverse of a matrix, and graphing. Some of these methods are easier to apply than others and are more appropriate in certain situations. In this section, we will study two more strategies for solving systems of equations.

Evaluating the determinant of a 2×2 matrix

A determinant is a real number that can be very useful in mathematics because it has multiple applications, such as calculating area, volume, and other quantities. Here, we will use determinants to reveal whether a matrix is invertible by using the entries of a square matrix to determine whether there is a solution to the system of equations. Perhaps one of the more interesting applications, however, is their use in cryptography. Secure signals or messages are sometimes sent encoded in a matrix. The data can only be decrypted with an invertible matrix and the determinant. For our purposes, we focus on the determinant as an indication of the invertibility of the matrix. Calculating the determinant of a matrix involves following the specific patterns that are outlined in this section.

Find the determinant of a 2 × 2 matrix

The determinant    of a 2   ×   2 matrix, given

A = [ a b c d ]

is defined as

Notice the change in notation. There are several ways to indicate the determinant, including det ( A ) and replacing the brackets in a matrix with straight lines, | A | .

Finding the determinant of a 2 × 2 matrix

Find the determinant of the given matrix.

A = [ 5 2 6 3 ]
det ( A ) = | 5 2 6 3 | = 5 ( 3 ) ( −6 ) ( 2 ) = 27
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Using cramer’s rule to solve a system of two equations in two variables

We will now introduce a final method for solving systems of equations that uses determinants. Known as Cramer’s Rule    , this technique dates back to the middle of the 18th century and is named for its innovator, the Swiss mathematician Gabriel Cramer (1704-1752), who introduced it in 1750 in Introduction à l'Analyse des lignes Courbes algébriques . Cramer’s Rule is a viable and efficient method for finding solutions to systems with an arbitrary number of unknowns, provided that we have the same number of equations as unknowns.

Cramer’s Rule will give us the unique solution to a system of equations, if it exists. However, if the system has no solution or an infinite number of solutions, this will be indicated by a determinant of zero. To find out if the system is inconsistent or dependent, another method, such as elimination, will have to be used.

To understand Cramer’s Rule, let’s look closely at how we solve systems of linear equations using basic row operations. Consider a system of two equations in two variables.

a 1 x + b 1 y = c 1 ( 1 ) a 2 x + b 2 y = c 2 ( 2 )

Questions & Answers

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Astronomy (from Ancient Greek ἀστρονομία (astronomía) 'science that studies the laws of the stars') is a natural science that studies celestial objects and phenomena. It uses mathematics, physics, and chemistry in order to explain their origin and evolution.
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these are Rocky substances between mars and jupiter
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Comets are cosmic snowballs of frozen gases , rock and dust that orbit the sun. They are mostly found between the orbits of Venus and Mercury.
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why the moon is always appear in an elliptical shape
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Because when astroid hit the Earth then a piece of elliptical shape of the earth was separated which is now called moon.
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Did you mean eye sight or sea level
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there are many theories regarding this it's on you believe any theory that you think is true ex. eternal inflation theory, oscillation model theory, multiple universe theory the big bang theory etc.
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in theory, you could see them all from the equator (though over the course of a year, not at pne time). stars are measured in "declination", which is how far N or S of the equator (90* to -90*). Polaris is the North star, and is ALMOST 90* (+89*). So it would just barely creep over the horizon.
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Source:  OpenStax, Algebra and trigonometry. OpenStax CNX. Nov 14, 2016 Download for free at https://legacy.cnx.org/content/col11758/1.6
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