Consider The Linear Transformation T From R3 To R2 With

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Kalali

Jun 15, 2025 · 3 min read

Consider The Linear Transformation T From R3 To R2 With
Consider The Linear Transformation T From R3 To R2 With

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    Understanding Linear Transformations from R³ to R²

    This article explores linear transformations, specifically focusing on a transformation T mapping vectors from a three-dimensional space (R³) to a two-dimensional space (R²). We'll delve into the concepts, explore how to represent such transformations using matrices, and examine some key properties. This will be useful for understanding linear algebra concepts in various applications, including computer graphics, data analysis, and machine learning.

    What is a Linear Transformation?

    A linear transformation is a function that maps vectors from one vector space to another while preserving vector addition and scalar multiplication. In simpler terms, it's a transformation that maintains the linear structure of the space. This means that for any vectors u and v in R³, and any scalar c:

    • T(u + v) = T(u) + T(v) (Additivity)
    • T(cu) = cT(u) (Homogeneity)

    Representing the Transformation with a Matrix

    A linear transformation from R³ to R² can always be represented by a 2x3 matrix. Let's say our transformation T maps the standard basis vectors of R³ – e₁ = (1, 0, 0), e₂ = (0, 1, 0), and e₃ = (0, 0, 1) – to vectors in R². The resulting vectors will determine the columns of our transformation matrix.

    Let's assume:

    • T(e₁) = (a, b)
    • T(e₂) = (c, d)
    • T(e₃) = (e, f)

    Then, the matrix representation of T is:

    A =  | a  c  e |
         | b  d  f |
    

    Any vector x = (x₁, x₂, x₃) in R³ can then be transformed by multiplying it with this matrix:

    T(x) = Ax

    This results in a vector in R². This matrix multiplication effectively performs the linear transformation.

    Example:

    Let's consider a specific example where:

    • T(e₁) = (1, 2)
    • T(e₂) = (0, 1)
    • T(e₃) = (-1, 0)

    The transformation matrix A would be:

    A =  | 1  0  -1 |
         | 2  1   0 |
    

    To transform the vector x = (3, 1, 2), we perform the matrix multiplication:

    | 1  0  -1 |   | 3 |   | 1 |
    | 2  1   0 | x | 1 | = | 3 |
                      | 2 |
    

    This gives us T(x) = (1, 5), which is a vector in R².

    Kernel and Range

    Two important concepts related to linear transformations are the kernel (null space) and the range (column space).

    • Kernel: The kernel of T is the set of all vectors in R³ that are mapped to the zero vector in R². It represents the vectors that are "annihilated" by the transformation. Finding the kernel involves solving the homogeneous system Ax = 0.

    • Range: The range of T is the set of all vectors in R² that are the image of some vector in R³. It represents the subspace of R² spanned by the columns of the transformation matrix A.

    Understanding the kernel and range provides valuable insights into the properties and behavior of the linear transformation.

    Conclusion:

    Linear transformations from R³ to R² provide a powerful tool for manipulating vectors and spaces. By understanding their matrix representation, we can perform calculations and analyze their properties. The kernel and range offer a deeper understanding of the transformation's effect on the input vectors. This framework has significant applications in numerous fields requiring vector manipulation and spatial transformations.

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