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Re: Projectile Launched Around the Earth
- To: mathgroup at smc.vnet.net
- Subject: [mg116431] Re: Projectile Launched Around the Earth
- From: "Ted Ersek" <ersekt at md.metrocast.net>
- Date: Tue, 15 Feb 2011 06:33:23 -0500 (EST)
The code below is n improved and more readable version of the demonstration
at
<http://demonstrations.wolfram.com/ProjectileLaunchedAroundTheEarth/>
http://demonstrations.wolfram.com/ProjectileLaunchedAroundTheEarth/
(*-----------------------------------------------------------------------*)
Manipulate[Module[{DiffEquations,ProjectilePosition,ProjectilePath,
EarthRadius,ProjectileCrashed,CrashSite,Projectile,Earth},
DiffEquations={D[x[t],t,t] == -4*Pi^2*x[t]*(x[t]^2+y[t]^2)^(-3/2),
D[y[t],t,t]==-4*Pi^2*y[t]*(x[t]^2+y[t]^2)^(-3/2),
x[0]==0,y[0]==y0,(x=92[0]==Vx0,(y=92[0]==0};
With[{DiffEqnSolution=NDSolve[DiffEquations, {x,y}, {t,0,t2}]},
ProjectilePosition[t_Real]={x[t],y[t]}/.DiffEqnSolution;
ProjectilePath=ParametricPlot[ ProjectilePosition[t], {t,0,t2},
PerformanceGoal->"Quality"];
ProjectileCrashed=MemberQ[ ProjectilePath, {_,_}?(Norm[#]<1&),
{6} ];
If[ProjectileCrashed,
ProjectilePath=ProjectilePath/.Line[pnts_]:>Line[ TakeWhile[
pnts, (1<Norm[#]&) ]];
CrashSite=Cases[ ProjectilePath,Line[pnts_]:>Last[pnts],-1];
Projectile=Graphics[{Red, PointSize[0.02], Point[CrashSite]
}],
(* else *)
Projectile=Graphics[{Red, PointSize[0.02],
Point[ProjectilePosition[t2]] }]
];
Earth=Graphics[{Gray,Disk[{0,0},1]}];
Show[ Earth, ProjectilePath, Projectile, PlotRange->4,
Axes->False] ]
],
{{t2, 2.9, "t"}, 0.01, 7.75},
{{y0, 1.4, "Subscript[y, 0]"}, 1.1, 3.97},
{{Vx0, 6.2, "Subscript[v, Subscript[x, 0]]"}, 1, 6.75}
]
(*--------------------------------------------------------------------------
------------------------------------*)
(*------How do we modify the code above to correctly model traveling around
the Earth? ----*)
When I tried to do it NDSolve complained that the equations were probably
stiff, and would not work it out automatically.
Note:
G = 6.672*^-11 (Newton (m/kg)^2)
EarthMass = 5.9721986=D710^24 kg
EarthRadius = 6378.14 km
F = G*EarthMass*ProjectileMass*(DistanceFromEarthCenter)^-2
Please indicate the units used for (t2, y0, Vx0)
Note:
EarthRadius above is the actual equatorial radius of the earth.
For simplicity we can model the earth as
a Sphere with(radius) = (actual equatorial radius).
I will ignore all complications such as wind resistance, variations in
density of the earth, etc.
Thanks,
Ted Ersek
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