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What Are the Key Equations That Describe Kinematics of Linear Motion?

When we start to learn about how things move in a straight line, it’s really important to understand some basic math formulas. Here are the main ones you need to know:

  1. What is Velocity?
    Average velocity (which we write as vavgv_{avg}) shows how fast something is moving. You can figure it out using this formula:
    vavg=ΔxΔtv_{avg} = \frac{\Delta x}{\Delta t}
    Here, Δx\Delta x is how far the object has moved, and Δt\Delta t is how long it took to move that distance.

  2. What is Acceleration?
    Acceleration (notated as aa) tells us how quickly something's speed is changing. It can be calculated with this formula:
    a=ΔvΔta = \frac{\Delta v}{\Delta t}
    In this case, Δv\Delta v is the change in speed.

  3. Equations of Motion:
    There are some important equations we use when acceleration stays the same. These are super helpful for figuring out problems:

    • First equation: v=u+atv = u + at
      (Here, uu is the starting speed)
    • Second equation: s=ut+12at2s = ut + \frac{1}{2}at^2
      (In this one, ss is how far the object has moved)
    • Third equation: v2=u2+2asv^2 = u^2 + 2as

These equations are great tools. They help us guess how an object will move when it speeds up or slows down at a steady rate. This makes them really useful for solving different kinds of problems in physics.

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What Are the Key Equations That Describe Kinematics of Linear Motion?

When we start to learn about how things move in a straight line, it’s really important to understand some basic math formulas. Here are the main ones you need to know:

  1. What is Velocity?
    Average velocity (which we write as vavgv_{avg}) shows how fast something is moving. You can figure it out using this formula:
    vavg=ΔxΔtv_{avg} = \frac{\Delta x}{\Delta t}
    Here, Δx\Delta x is how far the object has moved, and Δt\Delta t is how long it took to move that distance.

  2. What is Acceleration?
    Acceleration (notated as aa) tells us how quickly something's speed is changing. It can be calculated with this formula:
    a=ΔvΔta = \frac{\Delta v}{\Delta t}
    In this case, Δv\Delta v is the change in speed.

  3. Equations of Motion:
    There are some important equations we use when acceleration stays the same. These are super helpful for figuring out problems:

    • First equation: v=u+atv = u + at
      (Here, uu is the starting speed)
    • Second equation: s=ut+12at2s = ut + \frac{1}{2}at^2
      (In this one, ss is how far the object has moved)
    • Third equation: v2=u2+2asv^2 = u^2 + 2as

These equations are great tools. They help us guess how an object will move when it speeds up or slows down at a steady rate. This makes them really useful for solving different kinds of problems in physics.

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