183_notes:grav_pe_graphs

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183_notes:grav_pe_graphs [2021/04/01 16:57] – [Graphing Kinetic Energy] stumptyl183_notes:grav_pe_graphs [2024/01/31 14:45] (current) – hallstein
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 ==== Graphs of Gravitational Potential Energy ==== ==== Graphs of Gravitational Potential Energy ====
  
-[{{ 183_notes:grav_potential.png?400|A graph of the gravitational potential energy versus separation (solid red line); the zero of potential energy is marked with the solid black line.}}]+[{{ 183_notes:potentialgraph1_9.png?400|A graph of the gravitational potential energy versus separation (dashed purple line); the zero of potential energy is marked with the solid black line.}}]
  
 You can graph the gravitational potential energy (J) as a function of the radial separation, You can graph the gravitational potential energy (J) as a function of the radial separation,
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 For the figure on the right, the total energy is positive and hence, even at infinite distance, the less massive object has non-zero kinetic energy. This is an **unbound system** because the less massive object can move infinitely far away from the more massive object. For the figure on the right, the total energy is positive and hence, even at infinite distance, the less massive object has non-zero kinetic energy. This is an **unbound system** because the less massive object can move infinitely far away from the more massive object.
  
-[{{183_notes:k_plus_u_grav.001.png?525|A system where the total energy is overall negative because the magnitude of the gravitational potential energy is larger than the kinetic energy. This is a //bounded system//.}}] +[{{183_notes:potentialgraph2_9.png?525|A system where the total energy is overall negative because the magnitude of the gravitational potential energy is larger than the kinetic energy. This is a **bounded system.**}}] 
-[{{183_notes:k_plus_u_grav.002.png?525|A system where the total energy is overall positive because the magnitude of the gravitational potential energy is smaller than the kinetic energy. This is an //unbounded system//.}}]+[{{183_notes:potentialgraph3_9.png?525|A system where the total energy is overall positive because the magnitude of the gravitational potential energy is smaller than the kinetic energy. This is an** unbounded system**.}}]
  
  
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 ===== How is $\Delta U = mgh$ an approximation? ===== ===== How is $\Delta U = mgh$ an approximation? =====
  
-[{{183_notes:grav_potential_enlarged.png?500|The gravitational potential energy near the surface of the Earth (or any massive object) can be approximated as a linearly increasing function.}}]+[{{183_notes:potentialgraph4_9.png?500|The gravitational potential energy near the surface of the Earth (or any massive object) can be approximated as a linearly increasing function.}}]
  
 \\ \\
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 ==== Graphing Kinetic Energy ==== ==== Graphing Kinetic Energy ====
  
-[{{ 183_notes:grav_potential_kinetic.png?450|A graph of the potential, kinetic, and total energy of a gravitationally bound system. The kinetic energy is only for the less massive object in the system. The assumption is that it is much less massive than the larger object.}}]+[{{ 183_notes:potentialgraph5_9.png?450|A graph of the potential, kinetic, and total energy of a gravitationally bound system. The kinetic energy is only for the less massive object in the system. The assumption is that it is much less massive than the larger object.}}]
  
 It is often the the kinetic energy of the less massive object which is graphed along side the potential energy of the system and the total energy. For **a bound system**, this graph looks like the one to the right (green line is the kinetic energy).  It is often the the kinetic energy of the less massive object which is graphed along side the potential energy of the system and the total energy. For **a bound system**, this graph looks like the one to the right (green line is the kinetic energy). 
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 For an **unbound system** the kinetic energy levels off to the value of the total (positive) energy of the system. When the less massive object is infinitely far away, the potential energy of the system goes to zero. For an **unbound system** the kinetic energy levels off to the value of the total (positive) energy of the system. When the less massive object is infinitely far away, the potential energy of the system goes to zero.
  
 +/*
 ==== Examples ====  ==== Examples ==== 
  
   * [[:183_notes:examples:videoswk8|Video Example: Evaluating potential energy graphs (in an orbit)]]   * [[:183_notes:examples:videoswk8|Video Example: Evaluating potential energy graphs (in an orbit)]]
 +*/
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  • Last modified: 2021/04/01 16:57
  • by stumptyl