equations:newtons_second_law
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equations:newtons_second_law [2018/04/26 09:30] jakobadmin [Newton's Second Law] |
equations:newtons_second_law [2018/12/15 12:01] (current) 93.132.16.208 Small change in the previous edit |
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| However, take note that it is not sufficient to describe a physical system. Additionally, to describe a system we need to know what forces act on the object and what equations describe them. Famous examples of such force laws are | However, take note that it is not sufficient to describe a physical system. Additionally, to describe a system we need to know what forces act on the object and what equations describe them. Famous examples of such force laws are | ||
| - | * [[equations:newtons_law|Newton's law of gravity]] | + | * [[formulas:newtons_law|Newton's law of gravity]] |
| - | * [[equations:lorentz_force_law|Lorentz' force law]] | + | * [[formulas:lorentz_force_law|Lorentz' force law]] |
| - | * [[equations:coulombs_law|Coulomb's force law]] | + | * [[formulas:coulombs_law|Coulomb's force law]] |
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| - | So, for example, when we want to describe the movement of a planet around the sun we need to think about what forces act on the plant. For this system gravity is the most important force since both objects - the sun and the planet - a superheavy. Therefore, to calculate the movement of the planet, all we have to do is use [[equations:newtons_law|Newton's law of gravity]] to calculate the force acting on it. Then, when we have calculated the force we can use Newton's second law to calculate the acceleration of the object. Then, given some starting point and starting velocity of the planet we can calculate where the planet will be at every point in time in the future. | + | So, for example, when we want to describe the movement of a planet around the sun we need to think about what forces act on the plant. For this system gravity is the most important force since both objects - the sun and the planet - a superheavy. Therefore, to calculate the movement of the planet, all we have to do is use [[formulas:newtons_law|Newton's law of gravity]] to calculate the force acting on it. Then, when we have calculated the force we can use Newton's second law to calculate the acceleration of the object. Then, given some starting point and starting velocity of the planet we can calculate where the planet will be at every point in time in the future. |
| <tabbox Concrete> | <tabbox Concrete> | ||
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| + | **Boundary or Initial Conditions** | ||
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| + | Since Newton's second law contains the second derivative of the location: $\vec a = \frac{\partial^2 r}{\partial t^2}$, we need two boundary conditions to solve it. Whenever the independent variable is time, //boundary// conditions are usually called //initial// conditions. (In technical terms, we say that Newton's law is a second order differential equation.) For example, we can use the location of the object at the starting time and the velocity at the starting time as boundary conditions. Alternatively, we could use, for example, the location of the object at two different points in time as boundary conditions. | ||
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| **Example: The movement of an asteroid towards the sun** | **Example: The movement of an asteroid towards the sun** | ||
| - | As a first step, we use [[equations:newtons_law|Newton's law of gravity]] to calculate the force acting on the asteroid | + | As a first step, we use [[formulas:newtons_law|Newton's law of gravity]] to calculate the force acting on the asteroid |
| $$ F = G \frac{m_s m_a}{r^2},$$ | $$ F = G \frac{m_s m_a}{r^2},$$ | ||
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| - | Newton's second law is the most fundamental equation of [[theories:newtonian_mechanics|classical mechanics]]. It is still used nowadays, for example, by engineers. | + | Newton's second law is the most fundamental equation of [[theories:classical_mechanics:newtonian|classical mechanics]]. It is still used nowadays, for example, by engineers. |
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equations/newtons_second_law.1524727848.txt.gz · Last modified: 2018/04/26 07:30 (external edit)
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