NBC's Lester Holt looks at Newton's Third Law of Motion and the role that conservation of momentum plays whenever players collide on the football field. "Science of NFL Football" is a 10-part video series funded by the National Science Foundation and produced in partnership with the National Football League.
Science of NFL Football - Newton’s Third Law of Motion
LESTER HOLT, reporting:
Whether it's a lineman stuffing a running back or a safety colliding with a wide receiver, all NFL defenders have a single-minded goal - to stop the ball carrier.
HARDY NICKERSON (Former NFL Player): The object of making a tackle is you want to get the guy down and limit the amount of yards he’s able to gain, especially after contact.
HOLT: When a tackle is performed correctly, it's not just a thing of defensive beauty, it's also an elegant depiction of Newton's Third Law of Motion - sometimes called the "action-reaction" law.
TONY SCHMITZ (University of Florida): Newton’s Third Law say that each action or force has an equal and opposite reaction. So if I were to push against a body, that body is going to push back against me with an equal and opposite force.
HOLT: An important part of Newton's Third Law is the concept of momentum, which in football is the mass of a player, multiplied by his velocity, represented by the formula P equals MV. NFL players may not know the formula, but they're keenly aware of the role momentum plays in tackling.
NICKERSON: It’s very important to have some speed and momentum as you’re going in to make that tackle. The better you’re able to use that to your advantage, the better you’re able to make contact and get a guy down right away.
HOLT: In every collision on the football field, Newton's Third Law dictates that the total momentum between players must be the same before the collision as it is after the collision. This relationship is referred to as "Conservation of Momentum."
SCHMITZ: The Law of Conservation of Momentum says that the P, the momentum before the collision, is equal to P, the momentum after the collision.
HOLT: This law, represented by the formula P-before equals P-after (Pbefore=Pafter) can be illustrated with a simple toy called a "Newton's Cradle."
SCHMITZ: In this case, we have displaced an initial sphere and when we let it go, it has some momentum – it’s mass times velocity. When it impacts the next sphere that momentum is transferred through the middle three spheres and then passed onto the final sphere and so because it has the same mass, it will move away with the same velocity that the first sphere impacted the middle three spheres.
HOLT: The interaction of balls on a Newton's Cradle can help illustrate what's known as an "elastic collision," defined as one in which there is no loss of kinetic energy, in the form of heat, sound waves or deformation of the object. On the football field, collisions are typically "inelastic collisions" - because kinetic energy is released, mostly in the form of compression between the players' bodies and sound waves.
JIM GATES (University of Maryland): Inelastic collisions are the rule of the day. We see them all the time in football. That is the energy of motion of two runners after they collide, that energy is dissipated in deforming their bodies, that’s like a spring. So some of the energy of motion went into that compression. You might have heard a loud snap from our pads, some of the energy of our collision was transferred to the energy in the air that you hear.
HOLT: While big hits look and sound spectacular, what's most important in tackling is stopping the ball carrier's forward progress.
NICKERSON: If your pads are underneath his and you are hitting on the upward slope, you direct the energy up and take him back, at the point of contact, hopefully, that’s where the ball stops, play ends.
HOLT: Whether a tackle is successful or not, we can be certain that the same force is exerted on both players and the total momentum before and after the collision is the same. For that we have Newton's Third Law to thank.
Synopsis: Sir Isaac Newton developed the three basic Laws of Motion and stated the Law of Universal Gravitation, which together laid the foundation for our current understanding of physics and the Universe.
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