A remark on problem about trajectory of a projectile in the atmosphere

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The discussion highlights the well-known problem of projectile trajectory in the atmosphere, emphasizing the presence of a vertical asymptote. It presents the equations of motion for a projectile, incorporating factors such as gravitational force and atmospheric drag. The equilibrium state of the projectile is identified, demonstrating its exponential stability through the analysis of eigenvalues. As time progresses, the horizontal position stabilizes while the vertical position approaches a constant velocity. The conversation notes that various atmospheric drag models can be analyzed using stability theory, even when explicit integration is not feasible.
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This is just to share some teaching experience.
A problem about trajectory of a projectile in the atmosphere is very well known. The trajectory has a vertical asymptote. This fact is easy to obtain by using the stability theory.

Consider equations of motion. Let ##\boldsymbol v=v_x\boldsymbol e_x+v_y\boldsymbol e_y## be the velocity of the projectile relative the standard Earth fixed frame ##xy## with ##y## directed upwards.
The second Newton
##m\boldsymbol {\dot v}=m\boldsymbol g-\gamma |\boldsymbol v|\boldsymbol v;##
implies
##m\dot v_x=-\gamma v_x\sqrt{v_x^2+v_y^2},\quad \gamma=const>0,##
##m\dot v_y=-mg-\gamma v_y \sqrt{v_x^2+v_y^2}.##
This system has an equilibrium: ##v_x=0,\quad v_y=v^*:=-\sqrt{mg/\gamma}.##
This equilibrium is exponentially stable: eigenvalues of linearized system around this equilibrium are both negative so that
##v_x=O(e^{-c_x t}),\quad v_y=v^*+O(e^{-c_yt}),\quad c_x,c_y>0,\quad t\to\infty;##
and
##x(t)=x_0+\int_0^tv_xd\tau\to const,\quad y(t)\sim v^*t.##
Besides the quadratic model of atmosphere drag there are a lot of other models where the stability theory works but an explicit integration is impossible
 
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Why does the projectile’s velocity approach a constant value instead of increasing or decreasing indefinitely?
 
Each solution is bounded for ##t\ge 0##. This follows from the estimate
$$\frac{m}{2}\frac{d}{dt}|\boldsymbol v|^2=m(\boldsymbol g,\boldsymbol v)-\gamma|\boldsymbol v|^3\le m|\boldsymbol g||\boldsymbol v|-\gamma|\boldsymbol v|^3.$$
From the first equation we have
$$v_x(t)=v_x(0)e^{-\frac{\gamma}{m}\int_0^t|\boldsymbol v|d\tau}.$$
Thus ##v_x\to 0## as ##t\to \infty## and the
##\omega##-limit set of any solution belongs to the line ##\{v_x=0\}##. Only the set ##\{v_x=0,\quad v_y=v^*\}## is an invariant set that this line contains.
 
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