Friday, May 8, 2015

EJSS gravity 11

Example of Application of potential φ


Revision:  The total φ at a point in a field due to two or more source masses is the scalar addition of the individual φ due to each mass at that point, i.e.  .
φtotal = ∑ϕ
similarly, since PE = U = mφ
PE total = m  ϕ
Showing how the gravitational potential varies between the surface of the Moon and the surface of the Earth along the line joining the centres.

φ1 = Gravitational potential due to Moon

 φ2 = Gravitational potential due to Earth



φtotal = φ1 +φ2 = Net gravitational potential along the line of centres is equal to the sum of the gravitational potentials due to the Earth and Moon

work in progress: in an illustration scenario, the Masses M1 and M2 can be vary as well as their positions to provide a clearer example as shown below.

Escape Speed


Is it true that “what goes up must come down”?
It is only accurate to say that “what goes up may come down”.  There is a critical speed at which an object can be launched such that it can escape the Earth permanently.  Such a critical speed is termed as the escape speed.

Example


Determine an expression for the escape speed, v, of a rocket of mass m launched from the surface of Earth of mass M and radius R.

By conservation of energy, assuming at r = ∞, the minimum speed is 0.

KEearth surface + PEearth surface = KE + PE

1 2 m v 2 + ( - G m M r e a r t h ) = 0 + 0

1 2 v 2 + ( - ( 6.67 x 1 0 -11 ) ( 6.0 x 1 0 24 ) 6.37 x 1 0 6 ) = 0 + 0

v = 1.12x104 m/s

Therefore, to escape from Earth, it implies that the projectile must have a minimum velocity of v = 1.12x104 m/s .





To understand the escape velocity concept, the following steps could be used as an inquiry approach to experience escape velocity in the context of the simulation.

  1. uncheck the M1 moon to remove the effects of the Moon
  2. select from the drop-box menu the option Earth Surface view MoonEarth (Left to Right), and notice the test mass (red) is placed on the surface of the Earth on the right side.
  3. key in on the vtest, velocity of the test mass (magenta) say -10000 m/s (negative as the velocity shoot to the left of the Cartesian coordinate system)), and click play to observe the effects of launching a projectile at this speed. You could record your observation as "unable to escape from Earth's gravity pull.

similarly, design an experiment to discover the minimum theoretical speed to escape from Earth's pull.

can you conclude that any velocity lesser than v = 1.12x104 m/s cannot allow the projectile to escape from Earth's pull?

can you conclude that any velocity greater than vescape Earth = 1.12x104 m/s allow the projectile to escape from Earth's pull?


Similarly,  you can derive the theoretical escape velocity from Earth's Moon surface and test it on the simulation?
answer: vescape Moon=2400 m/s


given that root-mean-square speed is the measure of the speed of particles in a gas that is most convenient for problem solving within the kinetic theory of gases,  is given by v r m s = ( 3 R T M m )

Given gas constant R = 8.31 J K−1 mol−1, molar mass of water is Mm H20 = 18x10-3 kg/mol , T is temperature in Kelvin, using the minimum therotical speed from Moon, suggest the temperature of Moon surface at some point in its history where Moon surface does not have water.

T = 4.2x103 K

With this limited information, this data seems to suggest at some point of Moon's history, it could be very hot like T = 4.2x103 K and as the Moon cools, not enough water molecules was able to form on the Moon's surface to form oceans like what we have on Earth.

Java Model

http://iwant2study.org/lookangejss/02_newtonianmechanics_7gravity/ejs/ejs_model_GFieldandPotential1Dv7EarthMoon.jar

Model

https://dl.dropboxusercontent.com/u/44365627/lookangEJSworkspace/export/ejss_model_gravity11/gravity11_Simulation.xhtml